Members Can Post Anonymously On This Site
Sols 4229-4231: More Analyses of the Mammoth Lakes 2 Sample!
-
Similar Topics
-
By NASA
Curiosity Navigation Curiosity Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Mars Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions All Planets Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets 2 min read
Sols 4234-4235: And That’s (Nearly) a Wrap on Mammoth Lakes!
This image was taken by Mast Camera (Mastcam) onboard NASA’s Mars rover Curiosity on Sol 4219 (2024-06-19 02:21:12 UTC). Earth Planning Date: Wednesday, July 3, 2024
We received the data from our SAM analysis of the Mammoth Lakes sample late Monday afternoon. After chewing over the results, the team declared we are very happy with all of the analyses we’ve done with this sample, and we are ready to move on to greener pastures… er, redder rocks! This decision means that we will go ahead and clear out the drill assembly in today’s plan, and subsequently use the arm to collect MAHLI and APXS observations of the pile of drill tailings around the drill hole.
We’ll also have some time for remote sensing activities that use our mast-mounted instruments. Even though we’ve been parked at this location for several weeks, we’re still finding lots of things to look at! ChemCam will collect LIBS observations on a light-toned rock target named “Finger Peaks,” as well as a bumpy rock named “Glen Aulin.” We’ll also collect some additional Mastcam images of interesting features in the area, and a long-distance RMI mosaic of a target named “Rock Island Pass.” Several kinds of environmental monitoring activities will round out the plan.
It’s been a very productive drill sampling campaign here at Mammoth Lakes, our first after crossing into Gediz Vallis channel, and I’m excited to start getting ready to move on. What’s around the corner in this fascinating area of Mt. Sharp?
Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory
Share
Details
Last Updated Jul 03, 2024 Related Terms
Blogs Explore More
5 min read Sols 4232-4233: Going For a Ride, Anyone?
Article
2 days ago
2 min read Sols 4229-4231: More Analyses of the Mammoth Lakes 2 Sample!
Article
2 days ago
2 min read Sols 4226-4228: A Powerful Balancing Act
Article
6 days ago
Keep Exploring Discover More Topics From NASA
Mars
Mars is no place for the faint-hearted. It’s dry, rocky, and bitter cold. The fourth planet from the Sun, Mars…
All Mars Resources
Rover Basics
Mars Exploration Science Goals
View the full article
-
By NASA
Curiosity Navigation Curiosity Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Mars Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions All Planets Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets 5 min read
Sols 4232-4233: Going For a Ride, Anyone?
This image shows some of the sand ripples we spot all around the rover between the rocks. It was taken by Mast Camera (Mastcam) onboard NASA’s Mars rover Curiosity on Sol 4225 (2024-06-25 01:10:39 UTC). Earth planning date: Monday, July 1, 2024
Have you ever wondered what it might look like to ride along with the rover? Probably not as much as we have here on the planning team, where we are looking at the images on a daily basis. I always wish I could walk around there myself, or drive around in a vehicle, maybe. As you likely know, we don’t even get video, “just” images. But of course those images are stunning and the landscape is unique and – apart from being scientifically interesting – so very, very beautiful. And some cameras record images so often that it’s actually possible to create the impression of a movie. The front hazard camera is among them. And that can create a stunning impression of looking out of the front window! If you want to see that for yourself, you can! If you go to the NASA interactive tool called “Eyes on the Solar System” there is a Curiosity Rover feature that allows you to do just that: simulate a drive between waypoints and look out of the window, which is the front hazard camera. Here is the link to “Experience Curiosity.” The drive there is a while back, but the landscape is just so fascinating, I can watch and rewatch that any number of times!
Now, after reminiscing about the past, what did we do today? First of all: change all plans we ever had. We don’t have – as scheduled – the SAM data on Earth just yet. But we have a good portion of the sample still in the drill, and if SAM gets their data and wants to do more analysis with that sample, then we can’t move the arm as we originally had planned. Why didn’t we consider that to begin with? Normally, there isn’t enough sample for all the analysis; you may have seen this blog post: “Sols 4118-4119: Can I Have a Second Serving, Please? Oh, Me Too!” But it’s the sample that dictates how much we get to begin with, and how much we need, which only becomes clear as the data come in. And there is an unusually lucky combination here that would avoid us having to drill a second hole for getting the second helping. Instead, we just sit here carefully holding the arm still so we do not lose sample. That saves a lot of rover resources. But then, once we had settled how we adjust to keeping our current position, we also learnt that the uplink time might shift from the original slot we had been allocated to a later one… And all of this with a pretty new-to-the-role Science Operations Working Group (SOWG) chair (me) and a similarly new Geology and Mineralogy theme group science lead. Well, we managed, with lots of help from the great team around us.
Those sudden-change planning days are so tricky because there is so much more to remember. It’s not, “This is what we came to do…,” and it had been carefully pre-planned, and it is all in the notes. Instead, the pre-planning preparation doesn’t fit the new reality anymore, and all that work has to be redone. So we have to do all the pre-planning work, and the actual planning work, and sometimes also account for some “if… then…” scenarios in the same amount of time we usually have to do the planning on the basis of all the pre-planning work.
Sounds stressful? Yes, I can tell you it is!
Once we had changed all the skeleton plans, the team got very excited about the extra time. This is such an interesting area, there are rocks that are almost white, there are darker rocks, very interesting sand features with beautiful ripples, so much to look at! Mars has much to offer here, so the team got to work swiftly and the plan filled up with a great set of observations. ChemCam used LIBS on the target “Tower Peak,” which is one of those white-ish rocks, and on “Quarry Peak.” Mastcam delivers all the pictures to go along with these two activities and gets its own science, too. These are mainly so-called “change detection” images, where the same area is pictured repeatedly to see what particles might move in the time between the two images. ChemCam uses its long-distance imaging capability to add to the stunning images they are getting from faraway rocks. They have two mosaics on a target called “Edge Bench.” There is also a lot of atmospheric science in the plan; looking for dust devils and the opacity of the atmosphere are just two examples. REMS and DAN are also active throughout, to assess the wind, and the water underground, respectively. And as if that weren’t enough, CheMin also performs another night of analysis. We get to uplink a full plan, and we’ll see what the data say and what decisions we’ll make for next Wednesday.
Written by Susanne Schwenzer, Planetary Geologist at The Open University
Share
Details
Last Updated Jul 02, 2024 Related Terms
Blogs Explore More
2 min read Sols 4229-4231: More Analyses of the Mammoth Lakes 2 Sample!
Article
11 hours ago
2 min read Sols 4226-4228: A Powerful Balancing Act
Article
4 days ago
2 min read Interesting Rock Textures Galore at Bright Angel
Article
4 days ago
Keep Exploring Discover More Topics From NASA
Mars
Mars is no place for the faint-hearted. It’s dry, rocky, and bitter cold. The fourth planet from the Sun, Mars…
All Mars Resources
Rover Basics
Mars Exploration Science Goals
View the full article
-
By NASA
Curiosity Navigation Curiosity Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Mars Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions All Planets Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets 2 min read
Sols 4226-4228: A Powerful Balancing Act
NASA’s Mars rover Curiosity acquired this image about 10 inches (25 centimeters) from the “Loch Leven” target using its Mars Hand Lens Imager (MAHLI) close-up camera, located on the turret at the end of the rover’s robotic arm, in daylight on June 16, 2024, sol 4216 (or Martian day 4,216) of the Mars Science Laboratory Mission, at 05:12:12 UTC. Earth planning date: Tuesday, June 25, 2024
As documented in a previous blog last week, we continue to juggle power constraints as we focus on analyzing our newest drilled sample on Mars: “Mammoth Lakes 2.” Today, the star of the show is a planned dropoff to SAM (Sample Analysis at Mars instrument suite) and evolved gas analysis of the drill sample. This activity requires significant power so the team had to be judicious in planning other science observations and balancing the power needs of the different activities.
While the team eagerly awaits the outcome of the SAM and CheMin (Chemistry and Mineralogy X-Ray Diffraction instrument) analyses of Mammoth Lakes 2, we continue to acquire other observations in this fascinating area that will assist in our interpretations of the mineralogical data. ChemCam (the Chemistry and Camera instrument) will fire its laser at the “Loch Leven” target to get more chemical data on a target that was previously analyzed by APXS (the Alpha Particle X-Ray Spectrometer). “Loch Leven” is an example of gray material that rims the Mammoth Lakes drill block. The remote imaging capabilities of the ChemCam instrument will also be utilized to acquire a mosaic of a nearby area with interesting lighter- and darker-toned patches within the exposed rocks. Mastcam (Mast camera, for color stills and video) will document the ChemCam “Loch Leven” target and image the Mammoth Lakes 2 drill hole and surrounding fines to monitor any changes resulting from wind. We will also acquire extensions to two previous Mastcam mosaics: “Camp Four” and “Falls Ridge.”
To continue monitoring atmospheric conditions, the team also planned a Navcam (grayscale, stereoscopic Navigation cameras) large dust devil survey and Mastcam tau observation, an overhead image to measure dust in the atmosphere above Curiosity. Standard DAN (Dynamic Albedo of Neutrons instrument), REMS (Rover Environmental Monitoring Station), and RAD (Radiation Assessment Detector) activities round out the plan.
Written by Lucy Thompson, Planetary Geologist at University of New Brunswick
Share
Details
Last Updated Jun 27, 2024 Related Terms
Blogs Explore More
2 min read Interesting Rock Textures Galore at Bright Angel
Article
48 mins ago
2 min read Sol 4225: Sliding Down Horsetail Falls
Article
2 days ago
3 min read Sols 4222-4224: A Particularly Prickly Power Puzzle
Article
6 days ago
Keep Exploring Discover More Topics From NASA
Mars
Mars is no place for the faint-hearted. It’s dry, rocky, and bitter cold. The fourth planet from the Sun, Mars…
All Mars Resources
Rover Basics
Mars Exploration Science Goals
View the full article
-
By NASA
6 Min Read Surprising Phosphate Finding in NASA’s OSIRIS-REx Asteroid Sample
A microscope image of a dark Bennu particle, about a millimeter long, with a crust of bright phosphate. To the right is a smaller fragment that broke off. Credits: From Lauretta & Connolly et al. (2024) Meteoritics & Planetary Science, doi:10.1111/maps.14227. Early analysis of the asteroid Bennu sample returned by NASA’s OSIRIS-REx mission has revealed dust rich in carbon, nitrogen, and organic compounds, all of which are essential components for life as we know it. Dominated by clay minerals, particularly serpentine, the sample mirrors the type of rock found at mid-ocean ridges on Earth. The magnesium-sodium phosphate found in the sample hints that the asteroid could have splintered off from an ancient, small, primitive ocean world. The phosphate was a surprise to the team because the mineral had not been detected by the OSIRIS-REx spacecraft while at Bennu. While a similar phosphate was found in the asteroid Ryugu sample delivered by JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 mission in 2020, the magnesium-sodium phosphate detected in the Bennu sample stands out for its purity (that is, the lack of other materials included in the mineral) and the size of its grains, unprecedented in any meteorite sample. Scientists have eagerly awaited the opportunity to dig into the 4.3-ounce (121.6-gram) pristine asteroid Bennu sample collected by NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer) mission since it was delivered to Earth last fall. They hoped the material would hold secrets of the solar system’s past and the prebiotic chemistry that might have led to the origin of life on Earth. An early analysis of the Bennu sample, published June 26 in Meteoritics & Planetary Science, demonstrates this excitement was warranted.
The OSIRIS-REx Sample Analysis Team found that Bennu contains the original ingredients that formed our solar system. The asteroid’s dust is rich in carbon and nitrogen, as well as organic compounds, all of which are essential components for life as we know it. The sample also contains magnesium-sodium phosphate, which was a surprise to the research team, because it wasn’t seen in the remote sensing data collected by the spacecraft at Bennu. Its presence in the sample hints that the asteroid could have splintered off from a long-gone, tiny, primitive ocean world.
A Phosphate Surprise
Analysis of the Bennu sample unveiled intriguing insights into the asteroid’s composition. Dominated by clay minerals, particularly serpentine, the sample mirrors the type of rock found at mid-ocean ridges on Earth, where material from the mantle, the layer beneath Earth’s crust, encounters water.
This interaction doesn’t just result in clay formation; it also gives rise to a variety of minerals like carbonates, iron oxides, and iron sulfides. But the most unexpected discovery is the presence of water-soluble phosphates. These compounds are components of biochemistry for all known life on Earth today.
A tiny fraction of the asteroid Bennu sample returned by NASA’s OSIRIS-REx mission, shown in microscope images. The top-left pane shows a dark Bennu particle, about a millimeter long, with an outer crust of bright phosphate. The other three panels show progressively zoomed-in views of a fragment of the particle that split off along a bright vein containing phosphate, captured by a scanning electron microscope.From Lauretta & Connolly et al. (2024) Meteoritics & Planetary Science, doi:10.1111/maps.14227. While a similar phosphate was found in the asteroid Ryugu sample delivered by JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 mission in 2020, the magnesium-sodium phosphate detected in the Bennu sample stands out for its purity — that is, the lack of other materials in the mineral — and the size of its grains, unprecedented in any meteorite sample.
The finding of magnesium-sodium phosphates in the Bennu sample raises questions about the geochemical processes that concentrated these elements and provides valuable clues about Bennu’s historic conditions.
“The presence and state of phosphates, along with other elements and compounds on Bennu, suggest a watery past for the asteroid,” said Dante Lauretta, co-lead author of the paper and principal investigator for OSIRIS-REx at the University of Arizona, Tucson. “Bennu potentially could have once been part of a wetter world. Although, this hypothesis requires further investigation.”
“OSIRIS-REx gave us exactly what we hoped: a large pristine asteroid sample rich in nitrogen and carbon from a formerly wet world,” said Jason Dworkin, a co-author on the paper and the OSIRIS-REx project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
From a Young Solar System
Despite its possible history of interaction with water, Bennu remains a chemically primitive asteroid, with elemental proportions closely resembling those of the Sun.
“The sample we returned is the largest reservoir of unaltered asteroid material on Earth right now,” said Lauretta.
This composition offers a glimpse into the early days of our solar system, over 4.5 billion years ago. These rocks have retained their original state, having neither melted nor resolidified since their inception, affirming their ancient origins.
Hints at Life’s Building Blocks
The team has confirmed the asteroid is rich in carbon and nitrogen. These elements are crucial in understanding the environments where Bennu’s materials originated and the chemical processes that transformed simple elements into complex molecules, potentially laying the groundwork for life on Earth.
“These findings underscore the importance of collecting and studying material from asteroids like Bennu — especially low-density material that would typically burn up upon entering Earth’s atmosphere,” said Lauretta. “This material holds the key to unraveling the intricate processes of solar system formation and the prebiotic chemistry that could have contributed to life emerging on Earth.”
What’s Next
Dozens more labs in the United States and around the world will receive portions of the Bennu sample from NASA’s Johnson Space Center in Houston in the coming months, and many more scientific papers describing analyses of the Bennu sample are expected in the next few years from the OSIRIS-REx Sample Analysis Team.
“The Bennu samples are tantalizingly beautiful extraterrestrial rocks,” said Harold Connolly, co-lead author on the paper and OSIRIS-REx mission sample scientist at Rowan University in Glassboro, New Jersey. “Each week, analysis by the OSIRIS-REx Sample Analysis Team provides new and sometimes surprising findings that are helping place important constraints on the origin and evolution of Earth-like planets.”
Launched on Sept. 8, 2016, the OSIRIS-REx spacecraft traveled to near-Earth asteroid Bennu and collected a sample of rocks and dust from the surface. OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid, delivered the sample to Earth on Sept. 24, 2023.
NASA’s Goddard Space Flight Center in Greenbelt, Maryland, provided overall mission management, systems engineering, and the safety and mission assurance for OSIRIS-REx. Dante Lauretta of the University of Arizona, Tucson, is the principal investigator. The university leads the science team and the mission’s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft and provided flight operations. Goddard and KinetX Aerospace were responsible for navigating the OSIRIS-REx spacecraft. Curation for OSIRIS-REx takes place at NASA Johnson. International partnerships on this mission include the OSIRIS-REx Laser Altimeter instrument from CSA (Canadian Space Agency) and asteroid sample science collaboration with JAXA’s Hayabusa2 mission. OSIRIS-REx is the third mission in NASA’s New Frontiers Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington.
Find more information about NASA’s OSIRIS-REx mission at:
https://www.nasa.gov/osiris-rex
By Mikayla Mace Kelley
University of Arizona, Tuscon
News Media Contacts
Karen Fox / Erin Morton
NASA Headquarters, Washington
202-385-1287 / 202-805-9393
karen.c.fox@nasa.gov / erin.morton@nasa.gov
Rani Gran
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-332-6975
rani.c.gran@nasa.gov
Share
Details
Last Updated Jun 26, 2024 EditorRob GarnerLocationGoddard Space Flight Center Related Terms
OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer) Asteroids Astrobiology Astromaterials Bennu Goddard Space Flight Center Johnson Space Center Planetary Science The Solar System View the full article
-
By NASA
6 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The JunoCam instrument aboard NASA’s Juno spacecraft captured two volcanic plumes rising above the horizon of Jupiter’s moon Io. The image was taken Feb. 3 from a distance of about 2,400 miles (3,800 kilometers).Image data: NASA/JPL-Caltech/SwRI/MSSS, Image processing by Andrea Luck (CC BY) Infrared imagery from the solar-powered spacecraft heats up the discussion on the inner workings of Jupiter’s hottest moon.
New findings from NASA’s Juno probe provide a fuller picture of how widespread the lava lakes are on Jupiter’s moon Io and include first-time insights into the volcanic processes at work there. These results come courtesy of Juno’s Jovian Infrared Auroral Mapper (JIRAM) instrument, contributed by the Italian Space Agency, which “sees” in infrared light. Researchers published a paper on Juno’s most recent volcanic discoveries on June 20 in the journal Nature Communications Earth and Environment.
Io has intrigued the astronomers since 1610, when Galileo Galilei first discovered the Jovian moon, which is slightly larger than Earth. Some 369 years later, NASA’s Voyager 1 spacecraft captured a volcanic eruption on the moon. Subsequent missions to Jupiter, with more Io flybys, discovered additional plumes — along with lava lakes. Scientists now believe Io, which is stretched and squeezed like an accordion by neighboring moons and massive Jupiter itself, is the most volcanically active world in the solar system. But while there are many theories on the types of volcanic eruptions across the surface of the moon, little supporting data exists.
In both May and October 2023, Juno flew by Io, coming within about 21,700 miles (35,000 kilometers) and 8,100 miles (13,000 kilometers), respectively. Among Juno’s instruments getting a good look at the beguiling moon was JIRAM.
Infrared data collected Oct. 15, 2023, by the JIRAM instrument aboard NASA’s Juno shows Chors Patera, a lava lake on Jupiter’s moon Io. The team believes the lake is largely covered by a thick, molten crust, with a hot ring around the edges where lava from Io’s interior is directly exposed to space.NASA/JPL-Caltech/SwRI/ASI/INAF/JIRAM/MSSS Designed to capture the infrared light (which is not visible to the human eye) emerging from deep inside Jupiter, JIRAM probes the weather layer down to 30 to 45 miles (50 to 70 kilometers) below the gas giant’s cloud tops. But during Juno’s extended mission, the mission team has also used the instrument to study the moons Io, Europa, Ganymede, and Callisto. The JIRAM Io imagery showed the presence of bright rings surrounding the floors of numerous hot spots.
“The high spatial resolution of JIRAM’s infrared images, combined with the favorable position of Juno during the flybys, revealed that the whole surface of Io is covered by lava lakes contained in caldera-like features,” said Alessandro Mura, a Juno co-investigator from the National Institute for Astrophysics in Rome. “In the region of Io’s surface in which we have the most complete data, we estimate about 3% of it is covered by one of these molten lava lakes.” (A caldera is a large depression formed when a volcano erupts and collapses.)
Fire-Breathing Lakes
JIRAM’s Io flyby data not only highlights the moon’s abundant lava reserves, but also provides a glimpse of what may be going on below the surface. Infrared images of several Io lava lakes show a thin circle of lava at the border, between the central crust that covers most of the lava lake and the lake’s walls. Recycling of melt is implied by the lack of lava flows on and beyond the rim of the lake, indicating that there is a balance between melt that has erupted into the lava lakes and melt that is circulated back into the subsurface system.
This animation is an artist’s concept of Loki Patera, a lava lake on Jupiter’s moon Io, made using data from the JunoCam imager aboard NASA’s Juno spacecraft. With multiple islands in its interior, Loki is a depression filled with magma and rimmed with molten lava. NASA/JPL-Caltech/SwRI/MSSS “We now have an idea of what is the most frequent type of volcanism on Io: enormous lakes of lava where magma goes up and down,” said Mura. “The lava crust is forced to break against the walls of the lake, forming the typical lava ring seen in Hawaiian lava lakes. The walls are likely hundreds of meters high, which explains why magma is generally not observed spilling out of the paterae” — bowl-shaped features created by volcanism — “and moving across the moon’s surface.”
JIRAM data suggests that most of the surface of these Io hot spots is composed of a rocky crust that moves up and down cyclically as one contiguous surface due to the central upwelling of magma. In this hypothesis, because the crust touches the lake’s walls, friction keeps it from sliding, causing it to deform and eventually break, exposing lava just below the surface.
An alternative hypothesis remains in play: Magma is welling up in the middle of the lake, spreading out and forming a crust that sinks along the rim of the lake, exposing lava.
“We are just starting to wade into the JIRAM results from the close flybys of Io in December 2023 and February 2024,” said Scott Bolton, principal investigator for Juno at the Southwest Research Institute in San Antonio. “The observations show fascinating new information on Io’s volcanic processes. Combining these new results with Juno’s longer-term campaign to monitor and map the volcanoes on Io’s never-before-seen north and south poles, JIRAM is turning out to be one of the most valuable tools to learn how this tortured world works.”
Juno executed its 62nd flyby of Jupiter — which included an Io flyby at an altitude of about 18,175 miles (29,250 kilometers) — on June 13. The 63rd flyby of the gas giant is scheduled for July 16.
More About the Mission
NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. The Italian Space Agency (ASI) funded the Jovian InfraRed Auroral Mapper. Lockheed Martin Space in Denver built and operates the spacecraft.
More information about Juno is available at:
https://science.nasa.gov/mission/juno
News Media Contacts
DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov
Karen Fox / Charles Blue
NASA Headquarters
202-385-1287 / 202-802-5345
karen.c.fox@nasa.gov / charles.e.blue@nasa.gov
Deb Schmid
Southwest Research Institute, San Antonio
210-522-2254dschmid@swri.org
Share
Details
Last Updated Jun 26, 2024 Related Terms
Juno Jet Propulsion Laboratory Jupiter Jupiter Moons Explore More
5 min read Why Scientists Are Intrigued by Air in NASA’s Mars Sample Tubes
Article 6 days ago 2 min read Voyager 1 Returning Science Data From All Four Instruments
The spacecraft has resumed gathering information about interstellar space. NASA’s Voyager 1 spacecraft is conducting…
Article 2 weeks ago 4 min read NASA Announces New System to Aid Disaster Response
In early May, widespread flooding and landslides occurred in the Brazilian state of Rio Grande…
Article 2 weeks ago Keep Exploring Discover Related Topics
Missions
Humans in Space
Climate Change
Solar System
View the full article
-
-
Check out these Videos
Recommended Posts
Join the conversation
You can post now and register later. If you have an account, sign in now to post with your account.