Teachable Moments | August 16, 2024
Exploring the Next Frontier in Our Search for Life With Europa Clipper
Get the inside scoop on the Europa Clipper mission and its journey to explore an icy moon of Jupiter that could have conditions suitable for life. Plus, find ways to bring the excitement of the mission to your students.
In October, NASA's Europa Clipper mission will launch on a journey to investigate one of the next frontiers in our search for life beyond Earth. Its destination: Jupiter's moon Europa. Beneath its icy crust, the small moon is thought to contain a saltwater ocean with more water than all of Earth’s oceans combined. By studying the moon up close with a suite of scientific instruments, Europa Clipper aims to improve our understanding of the conditions on Europa and explore whether the moon could be suitable for life.
Read on to learn why scientists are so interested in this tiny ocean world and get to know the science behind the Europa Clipper mission. Then, follow along with the mission in the classroom using STEM teaching and learning resources.
Why Explore Europa?
In recent years, scientists have discovered likely water worlds throughout our solar system that might harbor conditions suitable for life. But scientists are especially intrigued by Jupiter's moon Europa because it hosts several components that make it one of the most promising for harboring a habitable environment.
Slightly smaller in size than Earth's Moon, Europa is one of Jupiter’s 95 officially recognized moons. Europa was discovered along with Jupiter's three other largest moons more than 400 years ago by astronomer Galileo Galilei, and named by astronomer Simon Marius, who discovered Europa around the same time.
Scientific observations of Europa by previous spacecraft, including the Galileo mission to Jupiter, point to the existence of a subsurface salty ocean. These observations included spectroscopic measurements indicating the surface is mostly water ice; gravitational and moment-of-inertia measurements indicating a layered internal structure, including a water and ice layer near the surface that is 62 miles (100 kilometers) thick; and magnetic field measurements indicating a conductive layer near the surface. A salty ocean would explain these observations.
Though Europa has been studied by the Galileo spacecraft and the more recent Juno spacecraft with a few up-close flybys, Europa Clipper will allow us to build on previous findings to gain new perspectives on the moon with a Europa-dedicated mission.
Europa’s surface is crisscrossed by long, linear fractures, cracks, ridges, and bands. This ice shell is probably 10 to 15 miles (15 to 25 kilometers) thick. Evidence suggests that below Europa’s icy surface there is a saltwater ocean that is about 25 times deeper than Earth's oceans and contains about twice as much water. Scientists are hopeful that the Europa Clipper mission will refine these estimates.
In addition to water, Europa could have other conditions needed for life as we know it, including chemistry, energy, and stability. NASA scientists believe that six essential chemical building blocks for life exist on Europa and have likely existed there since Europa formed. These common elements are carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur.
Chemical energy, similar to that produced by hydrothermal vents found on Earth’s ocean floor, may also exist on Europa’s sea floor. As Europa orbits Jupiter, it gets stretched and released by the tug of gravity from the giant planet. This process, called tidal flexing, creates heat, much in the same way a paperclip that is repeatedly bent back and forth can get hot to the touch. This tidal flexing process could keep the ocean liquid and may also be creating heat that could be released through hydrothermal vents on the ocean floor. On Earth, hydrothermal vents spew forth heated water, minerals, and various chemicals that react with the salty ocean, releasing stored chemical energy.
Radiation surrounding Jupiter is another possible source of fuel for life in an ocean below Europa's surface. Jupiter’s strong radiation bombards Europa, which is bad news for anything attempting to live on the surface. But the radiation splits apart water molecules at the surface. Once the water molecules are split, the hydrogen floats away into space and the oxygen stays behind, making it available to bind to other elements. If the oxygen makes its way to the ocean through cracks or openings, it could react with other chemicals to provide chemical energy for microbial life.
In addition to these potentially life-supporting conditions, observations indicate that the environment on Europa has likely remained constant for four billion years. Environmental stability is important to allow time for life to form and evolve. Such a promising stable environment is ripe for further exploration.
Europa Clipper Science
The Europa Clipper spacecraft will be the largest in NASA’s planetary mission history, measuring 16 feet (five meters) in height. Its giant solar arrays, the largest space-faring solar arrays to date, unfold in space to span the length of a basketball court, more than 100 feet (30.5 meters), and cover 950 square feet (90 square meters). Such an enormous light-collecting area is required because the intensity of the Sun near Jupiter is only 3% of what it is on Earth, and the massive arrays need to capture enough sunlight to power Clipper’s science instruments.
Europa Clipper has a powerful suite of nine science instruments designed to work together to study Europa’s surface features, improve our understanding of the moon’s icy shell, examine the interaction between the ocean and the icy shell, and investigate the ocean’s composition to determine if it has the ingredients to sustain life.
Exploring Europa’s Icy Surface
The spacecraft will collect images and generate surface maps using its onboard cameras and spectrometers which can identify chemical signatures from reflected light. The Europa Imaging System contains wide-angle and narrow-angle cameras, which will produce high-resolution color and stereoscopic images of Europa. These cameras will study Europa's geologic activity and measure surface elevations. The Europa Thermal Emission Imaging System will use infrared light to measure surface texture and characterize warmer regions where the liquid ocean may be closer to the surface. It will also show any visible evidence of water eruptions. The Europa Ultraviolet Spectrograph will use a telescope to collect ultraviolet light to help determine the makeup of Europa's sparse atmospheric gases and surface materials. It will also search for signs of plumes erupting from the surface.
A mass spectrometer and dust analyzer will measure the composition of tiny particles in Europa’s extremely thin atmosphere and surrounding environment. The mass spectrometer, or MASPEX, will analyze gases in Europa’s sparse atmosphere and in any plumes, as well as the chemical makeup of the ocean. The Surface Dust Analyzer will identify the chemistry of solid material ejected from Europa to offer clues about the surface composition and ocean salinity.
Examining Europa’s Icy Shell and Sub-surface Ocean
The spacecraft will search for water under Europa’s surface using radar and will gather magnetic field measurements with a magnetometer. An ice-penetrating radar instrument called REASON will examine the ice structure and thickness. It works by transmitting radio waves that bounce off of features within the ice, like cracks or pockets of water. By measuring the time difference between transmission and return, REASON will learn how far the features are from the spacecraft, and therefore, how deep they are in the ice. This highly specialized and advanced radar can also measure differences in the composition of materials on Europa. It does this by measuring the energy difference between transmitted and returning signals and combining them with distance measurements.
The Europa Clipper Magnetometer works by measuring small changes in Europa’s magnetic signal and how they vary with time and location. Measuring Europa’s magnetic signal could confirm the existence of an ocean and will help determine the ocean’s depth and salinity as well as the thickness of the moon's icy shell.
These instruments work in conjunction with several other instruments to closely study Europa during the flybys and return data for scientists to analyze for years to come. Explore a full list of instruments and learn how they work on the Europa Clipper mission website.
Getting to Europa
To save fuel for its journey to Europa, the spacecraft will follow what’s known as a Mars-Earth Gravity Assist trajectory for its 5.5-year journey. This path will first take the spacecraft near Mars to get a gravity assist – a boost in momentum obtained by tugging on Mars, thereby slightly decreasing Mars’ orbital momentum while transferring that momentum to the spacecraft. Next, Europa Clipper will swing back by Earth for another gravity assist before continuing on to Jupiter for its scheduled arrival in April 2030.
Once it arrives, Europa Clipper will orbit Jupiter in an elongated ellipse that will bring the spacecraft close to Europa about 50 times. The orbit was designed in this way to decrease the impact of Jupiter’s radiation on the spacecraft, which can damage its electronics. Studies show that a spacecraft orbiting Europa may survive for a few months, while one orbiting Jupiter would last for many years. After each close flyby of Europa, the spacecraft will travel outside Jupiter’s radiation belts to downlink data to Earth, uplink new commands, and prepare for the next flyby.
Follow Along
The Europa Clipper spacecraft is scheduled to launch in October 2024 from Kennedy Space Center in Florida. Tune in to watch the launch on NASA TV.
Visit the Europa Clipper mission website for all the latest mission updates, images, and science.
Teach Europa Clipper Science and Engineering
The Europa Clipper mission is a great opportunity to engage students with hands-on learning opportunities that range from imagining alien life forms to finding Jupiter in the night sky to engaging in the same science that led scientists to suspect the existence of Europa’s salty ocean. Explore these lessons and resources to get students excited about the STEM involved in this mission to determine if life-supporting conditions exist on Europa.
For Educators
For Students
Explore More
Activities for Kids
- Build Your Own Spacecraft Paper Model
- Build Your Own Spacecraft Toy Bricks Model
- Print a 3D Model of Europa Clipper
- Downloadable Europa Clipper
- Europa Clipper Mission Posters, Stickers, and More
Websites
Videos
Image Gallery
Articles
TAGS: K-12 Education, Educators, Teachers, Parents, Science, Astrobiology, Jupiter, Europa, Ocean, Teachable Moments
Edu News | January 16, 2024
Doing the Math on Why We Have Leap Day
Leap day, Feb. 29, happens every four years because of a mismatch between the calendar year and Earth's orbit. Learn how it works, and get students engaged in leap day STEM.
You may have noticed that there's an extra day on your calendar this year. That's not a typo – it's leap day! Leap day is another name for Feb. 29, a date that typically comes around every four years, during a leap year.
Why doesn't Feb. 29 appear on the calendar every year?
The length of a year is based on how long it takes a planet to revolve around the Sun. Earth takes about 365.2422 days to make one revolution around the Sun. That's about six hours longer than the 365 days that we typically include in a calendar year. As a result, every four years, we have about 24 extra hours that we add to the calendar at the end of February in the form of leap day.
Without leap day, the dates of annual events, such as equinoxes and solstices, would slowly shift to later in the year, changing the dates of each season. After only a century without leap day, summer wouldn’t start until mid-July!
But the peculiar adjustments don't end there. If Earth revolved around the Sun in exactly 365 days and six hours, this system of adding a leap day every four years would need no exceptions. However, Earth takes a little less time than that to orbit the Sun. Rounding up and inserting a 24-hour leap day every four years adds about 45 extra minutes to every four-year leap cycle. That adds up to about three days every 400 years. To correct for that, years that are divisible by 100 don't have leap days unless they’re also divisible by 400.
If you do the math, you'll see that the year 2000 was a leap year, but 2100, 2200 and 2300 will not be.
Have students learn more about leap years with this article from NASA's Space Place, then have them do the math for themselves with this leap day problem set. You can also have students write a letter or poem to be opened on the next leap day or get them learning about orbits across the solar system.
And since we've got an extra 24 hours this year, don't forget to take a little time to relax!
Educator Resources
- Problem Set
Leap Day Math
In this problem set, students calculate the difference between the calendar year and Earth's orbital period to determine when leap years occur.
Subject Math
Grades 5-8
Time Less than 30 mins
- Collection
Solar System Scale & Size Lessons
Explore a collection of standards-aligned lessons all about the size and scale of our solar system.
- Educator Guide
Planetary Poetry
Have students write a poem they can open and re-read next leap day!
Subject Science
Grades 2-12
Time 1-2 hrs
Student Resources
- Article
What Is a Leap Year?
Get the answer in this article from NASA Space Place. Plus, learn if other planets have leap years!
- Article
How Long Is a Year on Other Planets?
Get the answer in this article from NASA Space Place.
- Collection
All About the Size and Scale of the Solar System
Learn how big and far away the planets are with these projects and activities.
TAGS: K-12 Education, Math, Leap Day, Leap Year, Events, Space, Educators, Teachers, Parents, Students, STEM, Lessons, Earth Science, Earth
Edu News | August 17, 2023
Spend the School Year With NASA-JPL
Make educational connections to NASA and JPL happenings all year long with this calendar of upcoming events and links to educational resources you can use to explore STEM with us throughout the 2023-2024 school year.
August
All Month – Go Back to School With Us
The start of the school year is a great time to explore all of the resources we have on offer for educators, parents, and K-12 students. These include everything from classroom activities to DIY student projects to video tutorials to expert talks to our Teachable Moments series, which offers education-focused explainers of the latest NASA news.
There's something for every day of the school year, and you can find it all in one place on our Back to School event page. You can also sign up to receive monthly updates about new and featured content as well as upcoming events in your inbox with the JPL Education newsletter.
Learning Resources
- Public Event
Back to School With NASA-JPL Education
All the resources you'll need for a stellar school year from classroom lessons to student activities, challenges, and more!
- Sign Up
JPL Newsletter
Sign up to receive the latest STEM education resources, events, and news for teachers, students, and parents from the education team at JPL.
August 30 – See Supermoons on Parade
Skygazers will have plenty to moon over in August as the second of two supermoons this month graces the sky on August 30.
Make the event a Teachable Moment by dispelling common misconceptions about supermoons and digging into the real science behind the phenomena. Get students acting out moon phases, then have them apply what they've learned to make a Moon phases calendar and calculator. Plus, explore even more classroom activities and DIY projects all about our Moon.
Learning Resources
- Teachable Moments
What’s a Supermoon and Just How Super Is It?
Here’s what you can really expect to see during a supermoon. You don’t have to take our word for it. Get students investigating themselves.
- Collection
Moon Lessons for Educators
Teach students about the Moon with this collection of standards-aligned activities inspired by real NASA missions and science.
- Collection
Moon Activities for Students
Learn all about the Moon with these projects, slideshows, and videos for students.
September
September 24 – Follow Along as Asteroid Samples Arrive on Earth
Samples collected from the surface of an asteroid parachuted down to Earth on September 24, landing about 70 miles west of Salt Lake City. The samples were collected by the OSIRIS-REx spacecraft, which gathered the material during a daring descent on asteroid Bennu in 2018. The mission, which marks the first time the U.S. has collected samples from an asteroid, will give scientists an unparalleled, up-close look at remnants from our early solar system.
Follow along with the mission by having students do some of the same math as OSIRIS-REx mission planners. Or, have them do their own asteroid-related experiments. It's also a great opportunity to make connections to another NASA sample-return mission.
Learning Resources
- Collection
Asteroids Lessons for Educators
Explore a collection of standards-aligned lessons all about asteroids and craters.
- Collection
Asteroids Activities for Students
Explore projects, videos, slideshows, and games for students all about asteroids.
October
October 12 – Join NASA for the Psyche Launch
Did you know we can explore asteroids and other far away objects in the solar system to learn more about the interior of our own planet? That's one of the goals of NASA's Psyche mission, which is slated to launch on October 12 from NASA's Kennedy Space Center in Florida. The mission is designed to explore an asteroid – also named Psyche – that may be the remnant of a planet's core.
The Psyche spacecraft is one of just a handful of NASA missions throughout history that have used electric propulsion rather than a chemical engine, which means it's also a great opportunity to make connections to real-world examples of motion and forces. Get a primer on all the engineering and science behind the mission from our Teachable Moments series, then explore related lessons and projects.
Learning Resources
- Article
Teachable Moments: Asteroid Mission Aims to Explore Mysteries of Earth's Core
Explore how NASA's Psyche mission aims to help scientists answer questions about Earth and the formation of our solar system.
- Collection
Psyche Lessons for Educators
Explore a collection of standards-aligned lessons related to NASA's Psyche mission.
- Collection
Psyche Activities for Students
Explore projects, videos, slideshows, and games for students all about asteroids.
October 14 – Catch the Annular Solar Eclipse
October 14 marks the start of another exciting double-feature for skygazers: an annular solar eclipse followed by a total solar eclipse just six months later. In both events, the Sun, Moon, and Earth will align, creating a spectacular sight in the sky. But during the annular solar eclipse on October 14, a ring of sunlight will remain visible around the Moon. This is due to differences in the relative distances between the Sun, Moon, and Earth during the eclipse. In any case, remember to never look directly at the Sun without proper protection, such as certified solar eclipse glasses.
Another fun way to view a solar eclipse is by making a pinhole camera. Students can even use their pinhole cameras to make solar art. Check out our Teachable Moments article for more info on where and when to watch the eclipse, plus a primer on the science of solar eclipses. And explore even more eclipse lessons and activities – including a math puzzler from our NASA Pi Day Challenge.
Learning Resources
- Teachable Moment
The Science of Solar Eclipses and How to Watch With NASA
Get ready for the annular solar eclipse on Oct. 14, 2023. Learn about the science behind solar eclipses, how to watch safely, and how to engage students in NASA science.
- Student Project
How to Make a Pinhole Camera
Learn how to make your very own pinhole camera to safely see a solar eclipse in action!
- Lesson
Model a Solar Eclipse
Students use simple materials to model a partial, annular, and total solar eclipse.
- Math Problem
Eclipsing Enigma: A ‘Pi in the Sky’ Math Challenge
In this illustrated math problem, students use pi to figure out how much of the Sun’s disk will be covered by the Moon during an eclipse and whether it’s a total or annular eclipse.
Oct. 31 – Dare Mighty Pumpkins
Every Halloween, during an annual contest held at JPL, our engineers join kids and families across the country in the hallowed tradition of pumpkin carving. But these aren't your average jack-o'-lanterns. JPL pumpkins from years past have included a simulated Moon landing, Mars-themed whack-a-mole, and an exploding pumpkin supernova. The event, which takes place during employees' lunch break, gives all-new credence to the Lab's unofficial motto, "Dare Mighty Things." And it's good timing because this Halloween is also JPL's 87th birthday.
Whether history or Halloween are your thing, we've got ways to make educational connections – including a DIY project that gets students daring mighty pumpkins, themselves.
Learning Resources
- Collection
Halloween Activities for Students
Explore student projects and slideshows that put a Halloween twist on STEM.
- For Kids
Halloween Activities and Articles for Kids
Explore Halloween activities from NASA's Space Place, including pumpkin stencils, planet masks, an a scary space slideshow.
- Articles
Teachable Moments: JPL History
Explore key moments in JPL history and how they connect to what students are learning now.
November
All Month – Explore STEM Careers
Take part in National Career Development Month in November by exploring STEM opportunities at NASA and JPL. Students can learn more about careers in STEM and hear directly from scientists and engineers working on NASA missions in our Teaching Space video series. Meanwhile, our news page has more about what it takes to be a NASA astronaut and what it's like to be a JPL intern. You can also explore a collection of stories about NASA people, Women at NASA, and Women at JPL to learn more about the work they do.
For students already in college and pursuing STEM degrees, it's never too soon to start exploring internship opportunities for the summer. The deadline for JPL summer internships is March 29, so refresh your resume and get your application started now. Learn how to stand out with this article on how to get an internship at JPL – which also includes advice for pre-college students.
Learning Resources
- Expert Talks
Teaching Space With NASA
Hear from experts and education specialists about the latest missions and science happening at NASA and get your questions answered.
- Articles
Career Guidance
Get advice from scientists, engineers and educators about what it takes to work in science, technology, engineering and mathematics fields and how to get a foot in the door.
- Articles
Meet JPL Interns
These interns are pushing the boundaries of space exploration and science at the leading center for robotic exploration of the solar system.
- Opportunities
Internships and Jobs at JPL and NASA
Discover exciting opportunities at the leading NASA center for robotic exploration of the solar system.
December
All Month – Send Your Name to Jupiter
Here's a gift idea that doesn't cost a thing: Send a loved one's name to Jupiter with NASA's Europa Clipper mission. December is the last month to add your name to a microchip that will be flown on the spacecraft along with a poem written by the U.S. Poet Laureate, Ada Limón. The Europa Clipper mission, which is scheduled to launch in October 2024, is designed to explore Jupiter's ice-covered ocean moon Europa – the newest frontier in our search for life beyond Earth. So don't miss the boat – or, in this case, spacecraft – on this exciting opportunity.
Explore activities students can do in class or over winter break to write their own space poetry and engage in hands-on activities and experiments related to the Europa Clipper mission.
Learning Resources
- Collection
Europa Lessons for Educators
Explore classroom activities to bring the excitement of STEM and NASA's Europa Clipper mission to students.
- Collection
Europa Activities for Students
Learn all about Jupiter's moon Europa with these projects and videos for students.
- Public Event
Send Your Name to Jupiter
Have your name engraved on NASA's Europa Clipper spacecraft. Plus, explore more ways you can participate with the mission.
- Live Stream
Watch Engineers Build Europa Clipper Live at JPL
Get a live view into the "cleanroom" at NASA's Jet Propulsion Laboratory, where engineers are building the Europa Clipper spacecraft.
All Month – Prepare for the Science Fair
Before you know it, it'll be science fair time. Avoid the stress of science fair prep by getting students organized and thinking about their projects before the winter recess. Start by watching our video series How to Do a Science Fair Project. A scientist and an engineer from JPL walk your students through all the steps they will need to create an original science fair project by observing the world around them and asking questions.
You can also explore our science fair starter pack of lessons and projects to get students generating ideas and thinking like scientists and engineers.
Learning Resources
- Video Series
How to Do a Science Fair Project
Learn all the ins and outs of crafting your very own science fair project.
- Collection
Science Fair Lessons for Educators
Teach students how to craft their own science and engineering fair project with these video tutorials and lessons featuring NASA missions and science.
- Collection
Science Fair Activities for Students
Learn how to design a science and engineering fair project and get inspired with our catalog of student projects featuring NASA missions and science.
January
January 4 - Take a Closer Look at Jupiter's 'Pizza Moon'
Everyone's favorite pizza moon is getting another series of close-ups from NASA's Juno mission. Now that Juno has completed its primary science goals, mission planners are tweaking the spacecraft's orbit to send it past some of Jupiter's most fascinating moons. Io – notable for the more than 150 active volcanoes that splotch its surface like a bubbling cheese pizza – is next on the docket with two planned flybys this school year. Keep an eye on the mission website for updates and images from the first flyby on Dec. 30, 2023 that you can use to engage students before the second flyby on Feb. 3, 2024.
While on the topic of Juno, which holds the title of the most distant solar-powered spacecraft, it's a great opportunity to segue into math lessons involving pi, exponents, and the inverse square law. Or, highlight another record-holder: Rosaly Lopes, the JPL scientist who discovered 71 active volcanoes on Io, for which she was given the 2006 Guiness World Record for her discovery of the most active volcanoes anywhere.
Learning Resources
- Collection
Juno Lessons for Educators
Explore classroom activities to bring the excitement of STEM and NASA's Juno mission to students.
- Collection
Juno Activities for Students
Learn all about NASA's Juno mission with these projects, slideshows, and videos for students.
- Teachable Moments
Cruising to Jupiter: A Powerful Math Lesson
Find out how NASA’s Juno mission at Jupiter earned the title of most distant solar-powered spacecraft and how it relates to exponents.
February
February 18 – Learn What's Next for Mars Exploration
February 18 marks three years since NASA's Perseverance rover touched down on Mars, sticking the landing on one of the riskiest Red Planet descents to date. While the rover is coring away on Mars, collecting a diverse array of scientifically intriguing samples, mission teams here are busy designing, developing, and testing various devices to bring those samples to Earth. While we've collected samples from other objects in the solar system before (see October's asteroid sample return), this would be the first time we've retrieved samples from another planet. It requires an ambitious plan executed by multiple teams that need to achieve a number of other firsts – including the first launch from another planet.
Get students following along with classroom activities, projects, and challenges that have them apply their coding and collaboration skills to designing their own Mars sample return missions.
Learning Resources
- Collection
Mars Sample Return Lessons for Educators
Explore classroom activities to bring the excitement of STEM and NASA's Mars Sample Return mission to students.
- Collection
Mars Sample Return Activities for Students
Learn all about NASA's Mars Sample Return mission with these projects for students.
- Collection
Mission to Mars Student Challenge
Get K-12 students exploring Mars with NASA scientists, engineers, and the Perseverance rover as they learn all about STEM and design their very own mission to the Red Planet!
- Teachable Moments
NASA's Perseverance Rover Lands on Mars
Learn how, why, and what Perseverance will explore on Mars, plus find out about an exciting opportunity for you and your students to join in the adventure!
March
March 7-15 – Take the NASA Pi Day Challenge
There's more than pie to look forward to on March 14 as we'll be releasing an all-new set of Pi Day Challenge math problems involving NASA missions and science. Look for the latest problem set along with links to more resources and ways to celebrate Pi Day with us starting on March 7. You can get a sneak peek with the resources below, which work all year long, even without the slice of pie – although, we wouldn't blame you if you had one anyway.
Learning Resources
- Collection
Pi in the Sky Lessons
Find everything you need to bring the NASA Pi Day Challenge into the classroom, including printable handouts of each illustrated math problem.
- Student Project
NASA Pi Day Challenge
This collection of illustrated math problems gets students using pi like NASA scientists and engineers exploring Earth and space.
- Article
How Many Decimals of Pi Do We Really Need?
While you may have memorized more than 70,000 digits of pi, world record holders, a JPL engineer explains why you really only need a tiny fraction of that for most calculations.
- Article
18 Ways NASA Uses Pi
Whether it's sending spacecraft to other planets, driving rovers on Mars, finding out what planets are made of or how deep alien oceans are, pi takes us far at NASA. Find out how pi helps us explore space.
April
April 8 – Watch the Total Solar Eclipse
Time to get some solar eclipse glasses and dig out your pinhole cameras once again – this time for the headliner, a total solar eclipse on April 8. The eclipse will start in the South Pacific Ocean before passing over Mexico and following a diagonal path northeast over the U.S. and Canada. NASA is holding community events across the country where you can hear from speakers and participate in activities. Learn more on the agency's web page for all things solar eclipse.
Whether you're covering eclipse topics for the first time this school year or expanding on learning from October, this solar eclipse is a good time to get students exploring more about the science of eclipses. Start by looking at the five science experiments NASA has funded for the 2024 solar eclipse, then have students investigate solar eclipse science for themselves.
Learning Resources
- Teachable Moment
The Science of Solar Eclipses and How to Watch With NASA
Learn about the science behind solar eclipses, how to watch safely, and how to engage students in NASA science.
- Student Project
How to Make a Pinhole Camera
Learn how to make your very own pinhole camera to safely see a solar eclipse in action!
- Lesson
Model a Solar Eclipse
Students use simple materials to model a partial, annular, and total solar eclipse.
- Math Problem
Eclipsing Enigma: A ‘Pi in the Sky’ Math Challenge
In this illustrated math problem, students use pi to figure out how much of the Sun’s disk will be covered by the Moon during an eclipse and whether it’s a total or annular eclipse.
April 22 - Celebrate Earth Day With NASA
You may not immediately think of Earth science when you think of NASA, but it's a big part of what we do. Earth Day on April 22 is a great time to learn more about our Earth and climate science projects and missions, especially with the much anticipated NISAR mission taking to the skies in 2024 to track minute changes in the planet's surface, including those from natural hazards such as earthquakes, tsunamis, volcanoes and landslides.
Whether you want to focus on Earth’s surface and geology, climate change, extreme weather, or the water budget, we have an abundance of lessons, student projects and Teachable Moments to guide your way.
Learning Resources
- Collection
Earth Lessons for Educators
Discover a collection of standards-aligned STEM lessons all about Earth and climate change.
- Collection
Earth Activities for Students
Try these science and engineering projects, watch videos, and explore images all about the planet that we call home.
- Teachable Moments
Climate Change Collection
Explore this collection of Teachable Moments articles to get a primer on the latest NASA Earth science missions, plus find related education resources you can deploy right away!
May
May 6-10 – Give Thanks to Teachers and Black Holes
It may not seem like there's much to be gained from the dual programming of Black Hole Week and Teacher Appreciation Week on May 6-10, but sending students off to learn more about everyone's favorite spacely phenomenon might just give teachers the breather they deserve after a busy school year.
Have students dig into the science of black holes or even try out an experiment to learn how a black hole collision helped prove the existence of gravitational waves. Meanwhile, teachers can learn about all the ways their work has inspired us.
Learning Resources
- Slideshow
Black Holes: By the Numbers
What are black holes and how do they form?
- Lesson
Dropping In With Gravitational Waves
Students develop a model to represent the collision of two black holes, the gravitational waves that result and the waves' propagation through spacetime.
- Articles
Teachable Moments: Black Holes
Learn about the latest discoveries in black hole science and how to make connections to what students are learning.
- Share
Thank You, Teachers!
Employees at NASA's Jet Propulsion Laboratory give thanks to the teachers who helped them reach for the stars.
All Month – Launch Into Summer
Speaking of black holes, don't let students' learning fall into one as the summer gets into full swing. Send them off with links to these DIY summer projects. There's even more for parents and families on our Learning Space With NASA at Home page, which also has information to help direct students' learning during out-of-school time.
Learning Resources
- Student Resources
Summer Activities for Students
Explore Earth and space with these hands-on projects, slideshows, videos, and more for K-12 students.
- Student Resources
Learning Space With NASA
Explore space and science activities you can do with NASA at home. Find video tutorials, DIY projects, slideshows, games and more!
TAGS: Teachers, Classroom, Lessons, Educators, K-12, Parents, Students, Resources
Teachable Moments | August 16, 2023
Asteroid Mission Aims to Explore Mysteries of Earth's Core
Explore how NASA's Psyche mission aims to help scientists answer questions about Earth and the formation of our solar system. Then, make connections to STEM learning in the classroom.
NASA is launching a spacecraft in October 2023 to visit the asteroid Psyche, a metal-rich asteroid. The mission with the same name, Psyche, will study the asteroid, which is located in the main asteroid belt between Mars and Jupiter, to learn more about our solar system, including the core of our own planet.
Read more to find out what we will learn from the Psyche mission. Get to know the science behind the mission and follow along in the classroom using STEM teaching and learning resources from NASA.
Why It's Important
Asteroids are thought to be rocky remnants that were left over from the early formation of our solar system about 4.6 billion years ago. Of the more than 1.3 million known asteroids in our solar system, Psyche’s metallic composition makes it unique to study. Ground-based observations indicate that Psyche is a giant metal-rich asteroid about one-sixteenth the diameter of Earth’s Moon and shaped like a potato. Scientists believe it might be the partial nickel-iron core of a shattered planetesimal – a small world the size of a city that is the first building block of a planet. Asteroid Psyche could offer scientists a close look at the deep interiors of planets like Earth, Mercury, Venus, and Mars, which are hidden beneath layers of mantle and crust.
We can’t see or measure Earth’s core directly – it is more than 1,800 miles (3,000 kilometers) below the surface and we have only been able to drill about 7.5 miles (12 kilometers) deep with current technology. The pressure at Earth’s core measures about three million times the pressure of the atmosphere at the surface, and the temperature of Earth’s core is about 9,000 degrees Fahrenheit (5,000 degrees Celsius), so even if we could get science instruments there, the hostile conditions would make operations practically impossible. The Psyche asteroid may provide information that will allow us to better understand Earth’s core, including its composition and how it was created. The asteroid is the only known place in our solar system where scientists might be able to examine the metal from the core of a planetesimal.
The Psyche mission's science goals are to understand a previously unexplored building block of planet formation (iron cores); to explore a new type of world; and to look inside terrestrial planets, including Earth, by directly examining the interior of one of these planetary building blocks, which otherwise could not be seen. The science objectives that will help scientists meet these goals include determining if asteroid Psyche is actually leftover core material, measuring its composition, and understanding the relative age of Psyche's surface regions. The mission will also study whether small metal-rich bodies include the same light elements that are hypothesized to exist in Earth's core, determine if Psyche was formed under similar or different conditions than Earth's core, and characterize Psyche's surface features.
How It Will Work
The Psyche mission will launch on a SpaceX Falcon Heavy rocket. Psyche’s solar arrays are designed to work in low-light conditions because the spacecraft will be operating hundreds of millions of miles from the Sun. The twin plus-sign shaped arrays will deploy and latch into place about an hour after launch from Earth in a process that will take seven minutes for each wing. With the arrays fully deployed, the spacecraft will be about the size of a singles tennis court. The spacecraft’s distance from the Sun will determine the amount of power it can generate. At Earth, the arrays will be able to generate 21 kilowatts, which is enough electricity to power three average U.S. homes. While at asteroid Psyche, the arrays will produce about two kilowatts, which is a little more than what is needed to power a hair dryer.
The spacecraft will rely on the launch vehicle’s large chemical rocket engines to blast off the launchpad and escape Earth’s gravity, but once in space, the Psyche spacecraft will travel using solar-electric propulsion. Solar-electric propulsion uses electricity from the solar arrays to power the spacecraft’s journey to asteroid Psyche. For fuel, Psyche will carry tanks full of xenon, the same neutral gas used in car headlights and plasma TVs. The spacecraft’s four thrusters – only one of which will be on at any time – will use electromagnetic fields to accelerate and expel charged atoms, or ions, of that xenon. As those ions are expelled, they will create thrust that gently propels Psyche through space, emitting blue beams of ionized xenon. The thrust will be so gentle that it will exert about the same amount of pressure you’d feel holding three quarters in your hand, but it’s enough to accelerate Psyche through deep space. You can read more about ion propulsion in this Teachable Moment.
The spacecraft, which will travel 2.2 billion miles (3.6 billion kilometers) over nearly 6 years to reach its destination, will also use the gravity of Mars to increase its speed and to set its trajectory, or path, to intersect with asteroid Psyche’s orbit around the Sun. It will do this by entering and leaving the gravitational field of Mars, stealing just a little bit of kinetic energy from Mars’ orbital motion and adding it to its own. This slingshot move will save propellant, time, and expense by providing a trajectory change and speed boost without using any of the spacecraft’s onboard fuel.
Upon arrival at Psyche, the spacecraft will spend 26 months making observations and collecting data as it orbits the asteroid at different altitudes. Unlike many objects in the solar system that rotate like a spinning top, the asteroid Psyche rotates on its side, like a wheel. Mission planning teams had to take this unique characteristic into account in planning the spacecraft's orbits. The different orbits will provide scientists with ideal lighting for the spacecraft's cameras and they will enable the mission to observe the asteroid using different scientific instruments onboard.
The spacecraft will map and study Psyche using a multispectral imager, a gamma-ray and neutron spectrometer, a magnetometer, and a radio instrument (for gravity measurement). During its cruise to the asteroid, the spacecraft will also test a new laser communication technology called Deep Space Optical Communication, which encodes data in photons at near-infrared wavelengths instead of radio waves. Using light instead of radio allows the spacecraft to send more data back and forth at a faster rate.
Follow Along
Psyche is scheduled to launch no sooner than October 5, 2023 from Kennedy Space Center in Florida. Tune in to watch the launch on NASA TV.
Visit the mission website to follow along as data are returned and explore the latest news, images, and updates about this mysterious world.
Teach It
The Psyche mission is a great opportunity to engage students with hands-on learning opportunities. Explore these lessons and resources to get students excited about the STEM involved in the mission
Resources for Teachers
- Collection
Psyche Lessons for Educators
Explore a collection of standards-aligned lessons related to NASA's Psyche mission.
- Collection
Asteroids Lessons for Educators
Explore a collection of standards-aligned lessons all about asteroids and craters.
- Article
Teachable Moments: How NASA Studies and Tracks Asteroids Near and Far
Studying the chemical and physical properties, as well as the location and motion of asteroids, is vital to helping us understand how the sun, planets and other solar system bodies came to be. This article explores how NASA studies and tracks asteroids.
- Expert Talk
Teaching Space With NASA: Tracking Asteroids
In this educational talk, NASA experts will discuss how we track and study comets and asteroids. Plus, we'll answer your questions!
Activities for Students
-
Psyche Activities for Students
Explore projects, videos, slideshows, and games for students all about asteroids.
- Collection
Asteroids Activities for Students
Explore projects, videos, slideshows, and games for students all about asteroids.
Explore More
Resources for Kids
Check out these related resources for kids from NASA Space Place:
- Article for Kids: Asteroid or Meteor: What's the Difference?
- Article for Kids: What Is an Asteroid?
- Article for Kids: Why Does the Moon Have Craters?
- Article for Kids: What Is an Impact Crater?
Websites
Articles
Images
Videos
Interactives
Printouts
- Print a 3D Model of the Psyche Spacecraft
- Create a Psyche Lego Model
- Create a Model of the Psyche Asteroid
TAGS: Teachers, Classroom, Lessons, Educators, K-12, Parents, Students, Resources, Asteroid TM, Psyche
Teachable Moments | July 24, 2023
Exploring the Mystery of Our Expanding Universe
Learn about a new mission seeking to understand some of the greatest mysteries of our universe, and explore hands-on teaching resources that bring it all down to Earth.
Scientists may soon uncover new insights about some of the most mysterious phenomena in our universe with the help of the newly launched Euclid mission. Built and managed by the European Space Agency, Euclid will use a suite of instruments developed, in part, by NASA's Jet Propulsion Laboratory to explore the curious nature of dark energy and dark matter along with their role in the expansion and acceleration of our universe.
Read on to learn how the Euclid mission will probe these cosmological mysteries. Then, find out how to use demonstrations and models to help learners grasp these big ideas.
Why It’s Important
No greater question in our universe promotes wonder in scientists and non-scientists alike than that of the origin of our universe. The Euclid mission will allow scientists to study the nearly imperceptible cosmic components that may hold exciting answers to this question.
Edwin Hubble's observations of the expanding universe in the 1920s marked the beginnings of what's now known as the big-bang theory. We've since made monumental strides in determining when and how the big bang would have taken place by looking at what's known as cosmic background radiation using instruments such as COBE and WMAP in 1989 and 2001, respectively. However, there's one piece of Hubble's discovery that still has scientists stumped: our universe is not only expanding, but as scientists discovered in 1998, that expansion is also accelerating.
How can this be? It makes intuitive sense that, regardless of the immense force of the big bang that launched all matter across the known universe 13.8 billion years ago, that matter would eventually come to a rest and possibly even start to collapse. Instead, it's as if we've dropped a glass onto the ground and discovered that the shards are flying away from us faster and faster into perpetuity.
Scientists believe that answers may lie in two yet-to-be-understood factors of our universe: dark matter and dark energy. Dark matter is unlike the known matter we experience here on Earth, such as what's found on the periodic table. We can't actually see dark matter; we can only infer its presence. It has mass and therefore gravity, making it an attractive force capable of pulling things together. Amazingly, dark matter makes up roughly 27% of the known universe compared with the much more modest 5% of "normal matter" that we experience day to day. However, dark matter is extremely dilute throughout the universe with concentrations of 105 particles per cubic meter.
In opposition to the attractive force of dark matter, we have dark energy. Dark energy is a repulsive force and makes up roughly 68% of energy in the known universe. Scientists believe that the existence of dark energy and the amount of repulsion it displays compared with dark matter is what's causing our universe to not only expand, but also to expand faster and faster.
But to truly understand this mysterious force and how it interacts with both dark matter and normal matter, scientists will have to map barely detectable distortions of light traversing the universe, carefully measuring how that light changes over time and distance in every direction. As JPL Astrophysicist Jason Rhodes explains, “Dark energy has such a subtle effect that we need to survey billions of galaxies to adequately map it.”
And that's where Euclid comes in.
How It Works
The European Space Agency and NASA each contributed to the development of the Euclid mission, which launched from Cape Canaveral Space Force Station in Florida on July 1. The spacecraft consists of a 1.2-meter (48-inch) space telescope and two science instruments: an optical camera and a near-infrared camera that also serves as a spectrometer. These instruments will provide a treasure trove of data for scientists of numerous disciplines, ranging from exoplanet hunters to cosmologists.
As Gisella de Rosa at the Space Telescope Science Institute explains, “The ancillary science topics we will be able to study with Euclid range from the evolution of the objects we see in the sky today to detecting populations of galaxies and creating catalogs for astronomers. The data will serve the entire space community.”
The cameras aboard Euclid will operate at 530-920 nanometers (optical light) and at 920-2020 nanometers (near infrared) with each boasting more than 576 million and 65 million pixels, respectively. These cameras are capable of measuring the subtle changes to the light collected from celestial objects and can determine the distances to billions of galaxies across a survey of 15,000 square degrees – one-third of the entire sky.
Meanwhile, Euclid's spectrometer will collect even more detailed measurements of the distance to tens of millions of galaxies by looking at redshift. Redshift describes how wavelengths of light change ever so slightly as objects move away from us. It is a critical phenomenon for measuring the speed at which our universe is expanding. Similar to the way sound waves change as a result of the Doppler effect, wavelengths of light are compressed to shorter wavelengths (bluer) as something approaches you and extended to longer wavelengths (redder) as it moves away from you. As determined by a Nobel Prize winning team of astronomers, our universe isn’t just red-shifting over time, distant objects are becoming redder faster.
Euclid will measure these incredibly minuscule changes in wavelength for objects near and far, providing an accurate measurement of how the light has changed as a factor of time and distance and giving us a rate of acceleration of the universe. Furthermore, Euclid will be able to map the relative densities of dark matter and normal matter as they interact with dark energy, creating unevenly distributed pockets of more attractive forces. This will allow scientists to identify minute differences in where the universe is expanding by looking at the way that light is altered or "lensed."
The multi-dimensional maps created by Euclid – which will include depth and time in addition to the height and width of the sky – will inform a complementary mission already in development by NASA, the Nancy Grace Roman Space Telescope. Launching in 2026, this space telescope will look back in time with even greater detail, targeting areas of interest provided by Euclid. The telescope will use instruments with higher sensitivity and spatial resolution to peer deeper into redshifted and faint galaxies, building on the work of Euclid to look farther into the accelerating universe. As Caltech’s Gordon Squires describes it: “We’re trying to understand 90% of our entire universe. Both of these telescopes will provide essential data that will help us start to uncover these colossal mysteries.”
Teach It
The abstract concepts of the scope and origin of our universe and the unimaginable scale of cosmology can be difficult to communicate to learners. However, simple models and simulations can help make these topics more tangible. See below to find out how, plus explore more resources about our expanding universe.Resources
- Educator Guide
Model the Expanding Universe
Students learn about the role of dark energy and dark matter in the expansion of the universe, then make a model using balloons.
Subject Science
Grades 6-12
Time 30-60 mins
- Educator Guide
How Do We See Dark Matter?
Students will make observations of two containers and identify differences in content, justify their claims and make comparisons to dark matter observations.
Subject Science
Grades 6-12
Time Less than 30 mins
- Educator Guide
Math of the Expanding Universe
Students will learn about the expanding universe and the redshift of lightwaves, then perform their own calculations with a distant supernova.
Subject Science
Grades 9-12
Time 30-60 mins
- Collection
ViewSpace: Dark Energy Videos
Use this collection of short videos to introduce learners to the concept of dark energy.
- Collection
ViewSpace: Dark Matter Videos
Use this collection of short videos to introduce learners to the concept of dark matter.
- Science Briefing
Hubble Constant Discrepancies: Implications for Our Expanding Universe
Hear experts discuss how the rate of the universe is measured in different cosmological epochs and what the differences in those measures can tell us.
- Game
Roman Space Observer
How many astrophysical objects can you catch?
Explore More
- Article for Kids: What Is a Supernova?
- Article for Kids: What Is Dark Matter?
- Article: What Is Dark Energy?
- Article: Gravitational Lensing - Shining a Light on Dark Matter
- Facts & Figures: Euclid Mission - NASA
- Facts & Figures: Nancy Grace Roman Space Telescope
NASA's Universe of Learning materials are based upon work supported by NASA under award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and the Jet Propulsion Laboratory.
TAGS: K-12 Education, Teaching, Teachers, Educators, Resources, Universe, Dark Matter, Dark Energy, Euclid, Nancy Grace Roman Space Telescope, Universe of Learning
Teacher Feature | April 3, 2023
Working With the Next Wave of Science Teachers
Four pre-service teachers at Cal Poly Pomona are developing their skills in lesson design and delivery as they study Earth science concepts and prepare for graduation.
During the fall semester of 2022, I had the privilege of working with the Education Department at California Polytechnic University in Pomona, specifically with pre-service teachers taking coursework in Earth science. During our collaboration, the curriculum had the students split time in class between learning about geology and Earth’s history and then designing and engaging in classroom activities related to the technical content that they could take to their own classes in the future. This combination had Cal Poly students learning science and education hand-in-hand each week and led to some amazing classroom lessons and lab activities.
One group of young women in the program stood out as exceptionally passionate about their future careers. This team consisted of four seniors: Jacquelin Galvez-Coyt, hoping to someday teach kindergarten; Amie Gallardo, who is planning to teach fourth grade; Afiya Kindle, who is interested in teaching elementary or middle school; and Sofia Vallejo, who is interested in kindergarten through sixth grade.
Despite their interest in working with young students and collaborating to design lessons for those students, each of these pre-service teachers allowed their individuality to shape how they navigated lesson design and implementation. I recently sat down with them to ask about their instructional style and aspirations for classrooms of their own.
Now that we’re back to in-person classes, how is the transition going?
Sofia: Returning from remote instruction felt eerie at first, but it’s so nice to return to communicate with people and build connections in a non-digital way. In-person classes prepare you to communicate with colleagues in real life, build social skills, and read body language. All of these skills are critical for a teacher in order to understand and better help students to succeed.
Amie: Returning from remote instruction has been amazing. While it had its perks, I believe, as students, we learn a lot more while working hands-on with our projects than is possible in distance learning. If we’re trying to develop and assess activities we can do with kids, that really requires being face-to-face.
What are you most excited about when it comes to having your own classroom, and how will you get your kids excited about STEM?
Afiya: I am most confident about creating a genuine safe space for kids. I’ll be able to communicate how much I care about them and about our shared future, and I think there could never be enough genuinely kind and caring teachers in this world.
Jacquelin: I think my kids will be excited about STEM because of how easy it's become to incorporate activities. There are many resources out there for teachers to use for teaching math and science that don't rely solely on a textbook. Activities that use inexpensive materials or that require a little DIY skills go a long way for students.
Afiya: Exactly! I know I developed my love for science from being hands-on and actually somewhat “in charge” of an experiment on my own. Winning a science fair competition in seventh grade for a greenhouse I built really boosted my confidence and helped reassure me of my scholastic abilities as a kid.
You led a really cool lesson with your classmates where you had them use Oreos to model tectonic boundaries. How do you feel that lesson went?
Jacqueline: I was really proud of our group. After giving a lecture to the students about tectonic plate boundaries, we dispersed Oreos to everyone. We were set up around the classroom demonstrating the activity and giving verbal instructions for everyone to follow. My favorite part was when I saw two students by me go, “Oohhhh,” and smile once they got their Oreos to demonstrate the plate boundaries correctly.
Amie: I thought it went really well! All the students in our classroom enjoyed it. Although we, as adults, may know about plate tectonics, having our hands on the Oreos to understand it made it more enjoyable.
Afiya: Plus, who doesn’t love Oreos? They’re even vegan!
Which of the NASA-JPL lessons that you’ve implemented did you enjoy, and why?
Jacqueline: My favorite JPL activity we did was the Moon Phases activity. Having one team member to the side to give the instructions allows another student to view the different Moon phases. Then you switch so both students get to see that perspective. My second favorite activity was creating layers with different colored Play-Doh and demonstrating them as different plate boundaries and folds.
Amie: The NASA lesson that I enjoyed the most was the one we did on lunar eclipses. Much like myself, many students often have an early fascination with the Moon. Learning more about the Moon and lunar eclipses made me excited about the semester.
What’s next for you after you finish at Cal Poly Pomona?
Jacqueline: After I graduate at Cal Poly, I plan to attend UC Riverside to complete my credential program. While I am there, I would love to get my student teaching experience. Once I complete my credential program, I plan to apply to work at schools in the Inland Empire [in Southern California]. I want to be able to give back to the communities that influenced who I am today.
Sofia: My plans after Cal Poly are to take some time off to gain experience in the field as a substitute teacher. I also am looking to gain more volunteer experience, skills, and exposure. In the future, I want to enroll in UC Riverside to earn my teaching credential and master's degree.
Looking for ways to bring NASA STEM into your classroom or already have a great idea? The Education Office at NASA's Jet Propulsion Laboratory serves educators in the greater Los Angeles area. Contact us at education@jpl.nasa.gov.
Explore More
TAGS: Teachers, School, Remote School, Classroom, Instruction, K-12, STEAM, Science, Math, resources, lessons
Teachable Moments | January 3, 2023
How InSight Revealed the Heart of Mars
As NASA retires its InSight Mars lander, here's a look at some of the biggest discoveries from the first mission designed to study the Red Planet's interior – plus, how to make connections to what students are learning now.
After more than four years listening to the “heartbeat” of Mars, NASA is saying goodbye to the InSight lander as the mission on the Red Planet comes to an end. On Dec. 21, 2022 scientists wrapped up the first-of-its-kind mission to study the interior of Mars as dust in the Martian atmosphere and on the spacecraft’s solar panels prevented the lander from generating enough power to continue.
Read on to learn how the mission worked, what it discovered, and how to bring the science and engineering of the mission into the classroom.
How It Worked
The InSight lander was designed to reveal the processes that led to the formation of Mars – as well as Earth, the Moon, and all rocky worlds. This meant meeting two main science goals.
First, scientists wanted to understand how Mars formed and evolved. To do that, they needed to investigate the size and make-up of Mars’ core, the thickness and structure of its crust, the structure of the mantle layer, the warmth of the planet's interior, and the amount of heat flowing through the planet.
Second, to study tectonic activity on Mars, scientists needed to determine the power, frequency, and location of “marsquakes” as well as measure how often meteoroids impacted the Red Planet, creating seismic waves.
Engineers equipped InSight with three main science tools that would allow researchers to answer these questions about Mars.
SEIS, a seismometer like the ones used on Earth to record earthquakes, measured the seismic waves on Mars. These waves, which travel through the Red Planet, can tell scientists a lot about the areas they pass through. They even carry clues about whether it was a marsquake or meteorite impact that created the waves.
InSight's Heat Flow and Physical Properties Package, or HP3, was an instrument designed to burrow 16 feet (five meters) into Mars to measure the temperature at different depths and monitor how heat flowed out toward the surface. However, the self-hammering probe, informally called the "mole," struggled to dig itself in due to the unexpected consistency of the top few inches of Mars regolith at the landing site. Using full-size models of the lander and probe, engineers recreated InSight’s environment here on Earth to see if they could find a solution to the issue. They tested solutions that would allow the probe to penetrate the surface, including pressing the scoop attached to InSight’s robotic arm against the probe. While the effort serves as a great real-world example of how engineers work through problems with distant spacecraft, ultimately, none of the solutions allowed the probe to dig past the surface when attempted on Mars.
InSight’s third experiment, called RISE, used the spacecraft’s radio antennas to precisely measure the lander's position on the surface of Mars. The interior structure of Mars affects the planet’s motion, causing it to wobble. Measuring InSight’s position as the planet wobbled helped scientists gain a better understanding of the core and other layered structures that exist within the interior of Mars.
What We Discovered
InSight’s instruments enabled the mission science team to gain an understanding of not only the depth of Mars’ crust, mantle, and core, but also the composition of those features. They also learned just how active Mars really is.
The Structure of Mars
Working our way from the surface to the center of the planet, scientists found Mars’ crust was thinner than expected. Seismic waves detected by SEIS indicate that the crust is made up of three sub-layers, similar to Earth’s crust. The top-most layer of the crust is about six miles (10 kilometers) deep, while the denser layers of the crust, which contain more felsic, or iron-rich, material extend downward to about 25 miles (40 kilometers) below the surface. As seismic waves from a marsquake or a meteorite impact spread across the surface and through the interior of the planet, they can reflect off of underground layers, giving scientists views into the unseen materials below. Measuring how the waves change as a result of these reflections is how scientists unveiled the underground structure of Mars.
Like Earth, Mars has a lithosphere, a rigid layer made up of the crust and upper mantle. The Martian lithosphere extends about 310 miles (500 kilometers) below the surface before it transitions into the remaining mantle layer, which is relatively cool compared with Earth’s mantle. Mars’ mantle extends to 969 miles (1,560 kilometers) below the surface where it meets the planet’s core.
Scientists measured the core of Mars and found it to be larger than expected, with a radius of 1,137 miles (1,830 kilometers). With this information, scientists were able to estimate the density of Mars' core, which turned out to be less dense than anticipated, meaning it contains lighter elements mixed in with iron. Scientists also confirmed that the planet contains a liquid core. While we know that Earth has a liquid outer core and solid inner core, scientists will need to further study the data returned from InSight to know if there is also a solid inner core on Mars.
As scientists continue to study the data returned from InSight, we could learn even more about how Mars formed, how its magnetic field developed, and what materials make up the core, which could ultimately help us better understand how Earth and other planets formed.
Marsquakes
InSight discovered that Mars is a very active planet. A total of 1,319 marsquakes were detected after the SEIS instrument was placed on the surface. The largest, which was estimated to be a magnitude 5, was detected in May of 2022.
Unlike Earth, where the crust is broken into large pieces called plates that continually shift around causing earthquakes, Mars’ crust is made up of one solid plate, somewhat like a shell. However, as the planet cools, the crust shrinks, creating breaks called faults. This breaking action is what causes marsquakes, and the seismic waves generated by the quakes are what help scientists figure out when and where the quakes occurred and how powerful they were.
Nearly all of the strongest marsquakes detected by InSight came from a region known as Cerberus Fossae, a volcanic region that may have had lava flows within the past few million years. Volcanic activity, even without lava flowing on the surface, can be another way marsquakes occur. Images from orbiting spacecraft show boulders that have fallen from cliffs in this region, perhaps shaken loose by large marsquakes.
Conversely, InSight didn't detect any quakes in the volcanic region known as Tharsis, the home of three of Mars’ largest volcanos that sit approximately one-third of the way around the planet from InSight. This doesn’t necessarily mean the area is not seismically active. Scientists think there may be quakes occurring, but the size of Mars’ liquid core creates what’s known as a shadow zone – an area into which seismic waves don’t pass – at InSight's location.
Meteorite Impacts
On Sept. 5, 2021, InSight detected the impacts of a meteoroid that entered the Martian atmosphere. The meteoroid exploded into at least three pieces that reached the surface and left behind craters. NASA’s Mars Reconnaissance Orbiter passed over the impact sites to capture images of the three new craters and confirm their locations.
“After three years of waiting for an impact, those craters looked beautiful,” said Ingrid Daubar of Brown University, a Mars impacts specialist.
Mars’ thin atmosphere, which is less than 1% as dense as Earth’s, means meteoroids have a better chance of not disintegrating in the heat and pressure that builds up as they pass through the atmosphere to the planet’s surface. Despite this fact and Mars' proximity to the asteroid belt, the planet proved to be a challenging location to detect meteorite impacts because of "noise" in the data created by winds blowing on SEIS and seasonal changes in the atmosphere.
With the confirmation of the September 2021 impacts, scientists were able to identify a telltale seismic signature to these meteorite impacts. With this information in hand, they looked back through InSight's data and found three more impacts – one in 2020 and two in 2021. Scientists anticipate finding even more impacts in the existing data that might have been hidden by the noise in the data.
Meteorite impacts are an invaluable piece of understanding the planet’s surface. On a planet like Earth, wind, rain, snow and ice wear down surface features in a process known as weathering. Plate tectonics and active volcanism refresh Earth’s surface regularly. Mars’ surface is older and doesn't go through those same processes, so a record of past geologic events like meteorite impacts is more apparent on the planet's surface. By counting impact craters visible on Mars today, scientists can update their models and better estimate the number of impacts that occurred in the early solar system. This gives them an improved approximation of the age of the planet’s surface.
Why It's Important
Before InSight touched down, all Mars missions – landers, rovers, orbiters and flyby spacecraft – studied the surface and atmosphere of the planet. InSight was the first mission to study the deep interior of Mars.
Even with the InSight mission drawing to a close, the science and engineering of the mission will continue to inform our understanding of the Red Planet and our solar system for years as researchers further examine the data returned to Earth. Keep up to date with the latest findings from InSight scientists and engineers on the mission website.
Teach It
Explore these lessons in geology, physics, math, coding and engineering to connect student learning to the InSight mission and the real-world STEM that happens at NASA.
Educator Resources
- Collection
InSight Lessons for Educators
Explore a collection of standards-aligned lessons to bring the science and engineering of the InSight mission into the classroom.
- Collection
NASA's Mission to Mars Student Challenge
Get K-12 students exploring Mars with NASA scientists, engineers, and the Perseverance rover as they learn all about STEM and design their very own mission to the Red Planet!
- Teachable Moments
NASA InSight Lander to Get First Look at ‘Heart’ of Mars
Learn what it takes to travel to Mars and get students engaged with lessons in calculating trajectories, plus building and launching rockets.
- Teachable Moments
Mars Landing to Deliver Science Firsts
Find out how NASA’s InSight lander will collect all-new science at Mars, then get students doing similar investigations in the classroom.
Student Activities
Explore More
- Website: Mars InSight Mission
- Podcast: On a Mission - Season 1
- Articles: JPL News - InSight Mission
- Videos: InSight Mission Videos
- Images: InSight Mission Images
- Video: Interns Explore the Future at NASA-JPL
- Videos: Inside InSight - YouTube Playlist
- Videos: InSight Mission to Mars - YouTube Playlist
- Interactive: Experience InSight
- Website: NASA Mars Exploration
- Articles: People - Meet the Martians
- Resources for Kids: Space Place - All About Mars
TAGS: K-12 Education, Classrooms, Teaching, Teachers, Resources, Teachable Moments, Mars, InSight, Missions, Spacecraft, Marsquakes
Teachable Moments | December 8, 2022
NASA Mission Takes a Deep Dive Into Earth's Surface Water
Explore how and why the SWOT mission will take stock of Earth's water budget, what it could mean for assessing climate change, and how to bring it all to students.
Update: Dec. 15, 2022 – NASA, the French space agency, and SpaceX are now targeting 3:46 a.m. PST (6:46 a.m. EST) on Friday, Dec.16, for the launch of the Surface Water and Ocean Topography (SWOT) satellite. Visit NASA's SWOT launch blog for the latest updates.
NASA is launching an Earth-orbiting mission that will map the planet’s surface water resources better than ever before. Scheduled to launch on Dec. 16 from Vandenberg Space Force Base in California, the Surface Water and Ocean Topography, or SWOT mission is the latest international collaboration designed to monitor and report on our home planet. By providing us with a highly detailed 3D view of rivers, lakes, and oceans, SWOT promises to improve our understanding of Earth’s water cycle and the role oceans play in climate change, as well as help us better respond to drought and flooding.
Read on to find out why we're hoping to learn more about Earth's surface water, get to know the science behind SWOT's unique design, and follow along with STEM teaching and learning resources.
a name="swot_why">Why It's Important
Observing Earth from space provides scientists with a global view that is important for understanding the whole climate system. In the case of SWOT, we will be able to monitor Earth’s surface water with unprecedented detail and accuracy. SWOT will provide scientists with measurements of water volume change and movement that will inform our understanding of fresh water availability, flood hazards, and the mechanisms of climate change.
Water Flow
Scientists use a variety of methods to track Earth’s water. These include stream and lake gauges and even measurements from space such as sea surface altimetry and gravitational measurements of aquifer volumes. Monitoring of river flow and lake volume is important because it can tell us how much freshwater is readily available and at what locations. River flow monitoring can also help us make inferences about the downstream environmental impact. But monitoring Earth’s surface water in great detail with enough frequency to track water movement has proven challenging. Until now, most monitoring of river flow and lake levels has relied on water-flow and water-level gauges placed across Earth, which requires that they be accessible and maintained. Not all streams and lakes have gauges and previous space-based altimetry and gravitational measurements, though useful for large bodies of water, have not been able to adequately track the constant movement of water through smaller rivers or lakes.
SWOT will be able to capture these measurements across the globe in 3D every 21 days. The mission will monitor how much water is flowing through hundreds of thousands of rivers wider than 330 feet (100 meters) and keep a close watch on the levels of more than a million lakes larger than 15 acres (6 hectares). Data from the mission will be used to create detailed maps of rivers, lakes, and reservoirs that will enable accurate monitoring to provide a view of freshwater resources that is not reliant on physical access. Meanwhile, SWOT’s volumetric measurements of rivers, lakes, and reservoirs will help hydrologists better track drought and flooding impacts in near-real-time.
Coastal Sea Level Rise
SWOT will measure our oceans with unprecedented accuracy, revealing details of ocean features as small as 9 miles (15 kilometers) across. SWOT will also monitor sea levels and tides. Though we have excellent global sea level data, we do not have detailed sea level measurements near coastlines. Coastal sea levels vary across the globe as a result of ocean currents, weather patterns, land changes, and other factors. Sea levels are rising faster than ever, and higher sea levels also mean that hurricane storm surges will reach farther inland than ever before, causing substantially more damage than the same category of hurricanes in the past. SWOT will be able to monitor coastal sea level variations and fill gaps in the observations we currently have from other sources.
Ocean Heat Sinks
Further contributing to our understanding of the role Earth’s oceans play in climate change, SWOT will explore how the ocean absorbs atmospheric heat and carbon, moderating global temperatures and climate change. Scientists understand ocean circulation on a large scale and know that ocean currents are driven by temperature and salinity differences. However, scientists do not currently have a good understanding of fine-scale ocean currents, where most of the ocean's motion-related energy is stored and lost. Circulation at these fine scales is thought to be responsible for transporting half of the heat and carbon from the upper ocean to deeper layers. Such downward ocean currents have helped to mitigate the decades-long rise in global air temperatures by absorbing and storing heat and carbon away from the atmosphere. Knowing more about this process is critical for understanding the mechanisms of global climate change.
These fine-scale ocean currents also transport nutrients to marine life and circulate pollutants such as crude oil and debris. Understanding nutrient transport helps oceanographers assess ocean health and the productivity of fisheries. And tracking pollutants aids in natural hazard assessment, prediction, and response.
How It Works
A joint effort between NASA and the French space agency – with contributions from the Canadian and UK space agencies – SWOT will continue NASA’s decades-long record of monitoring sea surface height across the globe. But this mission will add a level of detail never before achieved.
SWOT will measure more than 90% of Earth’s surface water, scanning the planet between 78°N latitude and 78°S latitude within 1 centimeter of accuracy and retracing the same path every 21 days. Achieving this level of accuracy from a spacecraft height of 554 miles (891 kilometers) requires that the boom using radar to measure water elevation remain stable within 2 microns – or about 3% of the thickness of a human hair.
Prior to SWOT, spacecraft have used conventional nadir, or straight-down, altimetry to measure sea surface height. Conventional nadir altimetry sends a series of radar or laser pulses down to the surface and measures the time it takes for each signal to return to the spacecraft, thus revealing distances to surface features. To acquire more detailed information on surface water, SWOT will use an innovative instrument called the Ka-band Radar Interferometer, or KaRIn, to measure water height with exceptional accuracy. Ka-band is a portion of the microwave part of the electromagnetic spectrum. SWOT uses microwaves because they can penetrate clouds to return data about water surfaces.
The KaRIn instrument uses the principles of synthetic aperture radar combined with interferometry to measure sea surface height. A radar signal is emitted from the end of the 10-meter-wide boom on the spacecraft. The reflected signal is then received by antennas on both ends of the boom, capturing data from two 30-mile (50-kilometer) wide swaths on either side of the spacecraft. The received signals will be slightly out of sync, or phase, from one another because they will travel different distances to return to the receivers on either end of the boom. Knowing the phase difference, the distance between the antennas, and the radar wavelength allows us to calculate the distance to the surface.
The observations acquired by the two antennas can be combined into what is known as an interferogram. An interferogram is a pattern of wave interference that can reveal more detail beyond the 1-centimeter resolution captured by the radar. To explain how it works, we'll recall a couple of concepts from high school physics. When out-of-phase waves from the two antennas are combined, constructive and destructive interference patterns result in some wave crests being higher and some wave troughs being lower than those of the original waves. The patterns that result from the combination of the waves reveal more detail with resolution better than the 1-centimeter wavelength of the original Ka-band radar waves because the interference occurs over a portion of a wavelength. An interferogram can be coupled with elevation data to reveal a 3D representation of the water’s surface.
This highly accurate 3D view of Earth’s surface water is what makes SWOT so unique and will enable scientists to more closely monitor the dynamics of the water cycle. In addition to observing ocean currents and eddies that will inform our understanding of the ocean’s role in climate change, SWOT's use of interferometry will allow scientists to track volumetric changes in lakes and quantify river flooding, tasks that cannot yet be done on a wide scale in any other way.
Follow Along
SWOT is scheduled to launch no earlier than Dec. 16, 2022, on a SpaceX Falcon 9 rocket from Vandenberg Space Force Base in California. Tune in to watch the launch on NASA TV.
After launch, the spacecraft will spend 6-months in a calibration and validation phase, during which it will make a full orbit of Earth every day at an altitude of 553 miles (857 kilometers). Upon completion of this phase, SWOT will increase its altitude to 554 miles (891 kilometers) and assume a 21-day repeat orbit for the remainder of its mission.
Visit the mission website to follow along as data are returned and explore the latest news, images, and updates as SWOT provides a new view on one of our planet's most important resources.
Teach It
The SWOT mission is the perfect opportunity to engage students in studying Earth’s water budget and water cycle. Explore these lessons and resources to get students excited about the STEM involved in studying Earth’s water and climate change from space.
Educator Resources
- Collection
SWOT Mission Lessons for Educators
Explore the science and engineering behind the SWOT mission with this collection of standards-aligned lessons all about water.
- Collection
Climate Change Lessons for Educators
Explore a collection of standards-aligned STEM lessons for students that get them investigating climate change along with NASA.
- Collection
Teachable Moments in Climate Change
Explore this collection of Teachable Moments articles to get a primer on the latest NASA Earth science missions, plus find related education resources you can deploy right away!
- Expert Talk
Teaching Space With NASA – Monitoring Earth from Space
In this educational talk, NASA experts discuss how we build spacecraft to study climate, then answer audience questions.
Student Activities
- Collection
SWOT Mission Activities for Students
Explore projects, videos, slideshows, and games for students all about the water cycle and sea level rise.
- Collection
Climate Change Activities for Students
Learn about climate change and its impacts with these projects, videos, and slideshows for students.
- Collection
Earth Minute Video Series
This series of animated white-board videos for students of all ages explains key concepts about Earth science, missions, and climate change.
Explore More
Activities for Kids
- Download: SWOT Launch Bingo
- Video: How Much Water is on Earth?
- Game: Go With the Flow – An Ocean Currents Game
Websites
- SWOT Mission Website
- NASA Climate Change
- NASA Earth Observatory
- NASA Climate Kids
- NASA Sea Level Change
- NASA Cambio Climático en Español
Facts & Figures
Videos
Interactives
Image Gallery
Articles
- Climate articles from NASA
- Ask NASA Climate
- NASA People - Earth
- Water Mission to Gauge Alaskan Rivers on Front Lines of Climate Change
Podcast
TAGS: K-12 Education, Teachers, Educators, Earth Science, Earth, Climate Change, Climate, Satellites, Teachable Moments, Climate TM
Teachable Moments | October 20, 2022
The Science Behind NASA's First Attempt at Redirecting an Asteroid
Find out more about the historic first test, which could be used to defend our planet if a hazardous asteroid were discovered. Plus, explore lessons to bring the science and engineering of the mission into the classroom.
Update: Oct. 20, 2022 – The DART spacecraft successfully impacted the asteroid Dimorphos on September 26, reducing the period of the asteroid's orbit by 32 minutes. Scientists considered a change of 73 seconds to be the minimum amount for success. This article has been updated to reflect the latest data and images from the impact.
In a successful attempt to alter the orbit of an asteroid for the first time in history, NASA crashed a spacecraft into the asteroid Dimorphos on Sept. 26, 2022. The mission, known as the Double Asteroid Redirection Test, or DART, took place at an asteroid that posed no threat to our planet. Rather, it was an ideal target for NASA to test an important element of its planetary defense plan.
Read further to learn about DART, how it worked, and how the science and engineering behind the mission can be used to teach a variety of STEM topics.
Why It's Important
The vast majority of asteroids and comets are not dangerous, and never will be. Asteroids and comets are considered potentially hazardous objects, or PHOs, if they are 100-165 feet (30-50 meters) in diameter or larger and their orbit around the Sun comes within five million miles (eight million kilometers) of Earth’s orbit. NASA's planetary defense strategy involves detecting and tracking these objects using telescopes on the ground and in space. In fact, NASA’s Center for Near Earth Object Studies, or CNEOS, monitors all known near-Earth objects to assess any impact risk they may pose. Any relatively close approach is reported on the Asteroid Watch dashboard.
While there are no known objects currently posing a threat to Earth, scientists continue scanning the skies for unknown asteroids. NASA is actively researching and planning for ways to prevent or reduce the effects of a potential impact, should one be discovered. The DART mission was the first test of such a plan – in this case, whether it was possible to divert an asteroid from its predicted course by slamming into it with a spacecraft.
With the knowledge gained from the demonstration, similar techniques could be used in the future to deflect an asteroid or comet away from Earth if it were deemed hazardous to the planet.
How It Worked
With a diameter of about 525 feet (160 meters) – the length of 1.5 football fields – Dimorphos is the smaller of two asteroids in a double-asteroid system. Before DART's impact, Dimorphos orbited the larger asteroid called Didymos (Greek for "twin"), every 11 hours and 55 minutes.
Neither asteroid poses a threat to our planet, which is one reason why this asteroid system was the ideal place to test asteroid redirection techniques. At the time of DART's impact, the asteroid pair was 6.8 million miles (11 million kilometers) away from Earth as they traveled on their orbit around the Sun.
The DART spacecraft was designed to collide head-on with Dimorphos to alter its orbit, shortening the time it takes the small asteroid to travel around Didymos. Compared with Dimorphos, which has a mass of about 11 billion pounds (five billion kilograms), the DART spacecraft was light. It weighed just 1,210 pounds (550 kilograms) at the time of impact. So how did such a light spacecraft affect the orbit of a relatively massive asteroid?
DART was designed as a kinetic impactor, meaning it transferred its momentum and kinetic energy to Dimorphos upon impact, altering the asteroid's orbit in return. Scientists were able to make predictions about some of these effects thanks to principles described in Newton's laws of motion.
Newton’s first law told us that the asteroid’s orbit would remain unchanged until something acted upon it. Using the formula for linear momentum (p = m * v), we could calculate that the spacecraft, which at the time of impact would be traveling at 3.8 miles (6.1 kilometers) per second, would have about 0.5% of the asteroid’s momentum. The momentum of the spacecraft may seem small in comparison, but calculations suggested it would be enough to make a detectable change in the speed of Dimorphos' orbit. However, mission planners felt that changing Dimorphos’ orbit by at least 73 seconds would be enough to consider the test a success.
But there was more to consider in testing whether the technique could be used in the future for planetary defense. For example, the formula for kinetic energy (KE = 0.5 * m * v2) tells us that a fast moving spacecraft possesses a lot of energy.
When DART hit the surface of the asteroid, its kinetic energy was 10 billion joules! A crater was formed and material known as ejecta was blasted out as a result of the impact. Scientists are still studying the data returned from the mission to determine the amount of material ejected out of the crater, but estimates prior to impact put the number at 10-100 times the mass of the spacecraft itself. The force needed to push this material out was then matched by an equal reaction force pushing on the asteroid in the opposite direction, as described by Newton’s third law.
How much material was ejected and its recoil momentum is still unknown. A lot depends on the surface composition of the asteroid, which scientists are still investigating. Laboratory tests on Earth suggested that if the surface material was poorly conglomerated, or loosely formed, more material would be blasted out. A surface that was well conglomerated, or densely compacted, would eject less material.
After the DART impact, scientists used a technique called the transit method to see how much the impact changed Dimorphos' orbit. As observed from Earth, the Didymos pair is what’s known as an eclipsing binary, meaning Dimorphos passes in front of and behind Didymos from our view, creating what appears from Earth to be a subtle dip in the combined brightness of the pair. Scientists used ground-based telescopes to measure this change in brightness and calculate how quickly Dimorphos orbits Didymos. By comparing measurements from before and after impact, scientists determined that the orbit of Dimorphos had slowed by 32 minutes to 11 hours and 23 minutes.
One of the biggest challenges of the DART mission was navigating a small spacecraft to a head-on collision with a small asteroid millions of miles away. To solve that problem, the spacecraft was equipped with a single instrument, the DRACO camera, which worked together with an autonomous navigation system called SMART Nav to guide the spacecraft without direct control from engineers on Earth. About four hours before impact, images captured by the camera were sent to the spacecraft's navigation system, allowing it to identify which of the two asteroids was Dimorphos and independently navigate to the target.
DART was not just an experimental asteroid impactor. The mission also used cutting-edge technology never before flown on a planetary spacecraft and tested new technologies designed to improve how we power and communicate with spacecraft.
One such technology that was first tested on the International Space Station and was later used on the solar-powered DART spacecraft, is the Roll Out Solar Array, or ROSA, power system. As its name suggests, the power system consisted of flexible solar panel material that was rolled up for launch and unrolled in space.
Some of the power generated by the solar array was used for another innovative technology, the spacecraft's NEXT-C ion propulsion system. Rather than using traditional chemical propulsion, DART was propelled by charged particles of xenon pushed from its engine. Ion propulsion has been used on other missions to asteroids and comets including Dawn and Deep Space 1, but DART's ion thrusters had higher performance and efficiency.
Follow Along
In the days following the event, NASA received images of the impact from a cubesat, LICIACube, that was deployed by DART before impact. The cubesat, which was provided by the Italian Space Agency, captured images of the impact and the ejecta cloud.
Meanwhile, the James Webb Space Telescope, the Hubble Space Telescope, and the Lucy spacecraft observed Didymos to monitor how soon reflected sunlight from the ejecta plume could be seen. Going forward, DART team members will continue observing the asteroid system to measure the change in Dimorphos’ orbit and determine what happened on its surface. And in 2024, the European Space Agency plans to launch the Hera spacecraft to conduct an in-depth post-impact study of the Didymos system.
Continue following along with all the science from DART, including the latest images and updates on the mission website.
Teach It
The mission is a great opportunity to engage students in the real world applications of STEM topics. Start exploring these lessons and resources to get students engaging in STEM along with the mission.
Educator Guides
Expert Talks
Student Activities
Articles
- Teachable Moments
How NASA Studies and Tracks Asteroids Near and Far
Here’s how NASA uses math and science to track the movements of asteroids and find out what they’re made of – and students can, too.
- Meet JPL Interns
From Island Life to Spotting Asteroids for NASA
Meet a JPL intern whose journey took her from the remote island of Saipan to a team helping track asteroids at NASA.
Resources for Kids
Check out these related resources for kids from NASA Space Place:
- Article for Kids: Asteroid or Meteor: What's the Difference?
- Article for Kids: What Is an Asteroid?
- Article for Kids: Why Does the Moon Have Craters?
- Article for Kids: What Is an Impact Crater?
Explore More
- Facts & Figures: Didymos In Depth
- Facts & Figures: DART Mission
- Website: DART Mission
- Gallery: DART Mission Images and Videos
- Facts & Figures: Asteroid Watch
- Gallery: Next Five Asteroid Approaches
- Articles: Asteroid News and Images from JPL
- Eyes on Asteroids
- Eyes on the Solar System - DART Impact
- Quiz: Are You a Planetary Defnder?
- Center for Near-Earth Object Studies
TAGS: Asteroids and Comets, DART, near-Earth objects, planetary defense, Science, K-12 Education, Teachers, Educators, Parents, Teachable Moments, Asteroid TM