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Looking Out for ‘Lookout Hill’
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By NASA
NASA/Shawn Quinn On May 8, 2022, NASA’s Exploration Ground Systems’ Program Manager Shawn Quinn captured this crop of a full frame image of the Hadley–Apennine region of Earth’s Moon including the Apollo 15 landing site (very near the edge of the shadow of one of the lunar mountains in the area). Building upon the pioneers from the Apollo Program, Artemis crews will plan to verify capabilities for humans to explore deep space and pave the way for long-term exploration and science on the lunar surface.
Read the Artemis blog for the latest mission updates.
Image credit: NASA/Shawn Quinn
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By Space Force
Guardians connected with members of Congress at a special screening of "The U.S. Space Force — America's Invisible Front Line" documentary at the U.S. Capitol Visitor Center April 30, 2025.
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By NASA
Explore This Section Perseverance Home Mission Overview Rover Components Mars Rock Samples Where is Perseverance? Ingenuity Mars Helicopter Mission Updates Science Overview Objectives Instruments Highlights Exploration Goals News and Features Multimedia Perseverance Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 2 min read
Origins Uncertain: ‘Skull Hill’ Rock
Written by Margaret Deahn, Ph.D. Student at Purdue University
Last week, NASA’s Mars 2020 rover continued its journey down lower ‘Witch Hazel Hill’ on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called ‘Port Anson’. In addition to this contact, the rover has encountered a variety of neat rocks that may have originated from elsewhere and transported to their current location, also known as float.
This image from NASA’s Mars Perseverance rover, taken by the Mastcam-Z instrument’s right eye, shows the ‘Skull Hill’ target, a dark-toned float rock. The rover acquired this image while driving west downslope towards lower ‘Witch Hazel Hill’. Perseverance acquired this image on April 11, 2025, or sol 1472 of the Mars 2020 mission NASA/JPL-Caltech/ASU Pictured above is an observation named ‘Skull Hill’ taken by the rover’s Mastcam-Z instrument. This float rock uniquely contrasts the surrounding light-toned outcrop with its dark tone and angular surface, and it features a few pits in the rock. If you look closely, you might even spot spherules within the surrounding regolith! See Alex Jones’ recent blog post for more information on these neat features: https://science.nasa.gov/blog/shocking-spherules/. The pits on Skull Hill may have formed via the erosion of clasts from the rock or scouring by wind. We’ve found a few of these dark-toned floats in the Port Anson region, and the team is working to better understand where these rocks came from and how they got here.
Skull Hill’s dark color is reminiscent of meteorites found in Gale crater by the Curiosity rover: https://www.jpl.nasa.gov/news/curiosity-mars-rover-checks-odd-looking-iron-meteorite/. Chemical composition is an important factor in identifying a meteorite, and Gale’s meteorites contain significant amounts of iron and nickel. However, recent analysis of SuperCam data from nearby similar rocks suggests a composition inconsistent with a meteorite origin.
Alternatively, ‘Skull Hill’ could be an igneous rock eroded from a nearby outcrop or ejected from an impact crater. On Earth and Mars, iron and magnesium are some of the main contributors to igneous rocks, which form from the cooling of magma or lava. These rocks can include dark-colored minerals such as olivine, pyroxene, amphibole, and biotite. Luckily for us, the rover has instruments that can measure the chemical composition of rocks on Mars. Understanding the composition of these darker-toned floats will help the team to interpret the origin of this unique rock!
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Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 2 min read
Sols 4493-4494: Just Looking Around
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on March 25, 2025 — sol 4491, or Martian day 4,491 of the Mars Science Laboratory mission — at 17:16:50 UTC. NASA/JPL-Caltech Written by Alex Innanen, atmospheric scientist at York University
Earth planning date: Wednesday, March 26, 2025
It’s my second shift of the week as the Environmental theme lead and keeper of the plan (a bit of a mouthful we shorten to ESTLK) and today started out feeling eerily similar to Monday. Once again, Curiosity is posing like a geologist, which means that once again we can’t unstow the arm and will be skipping contact science. The silver lining is that this means we have extra time to have a good look around.
The plan also looks similar to Monday’s — targeted remote sensing on the first sol before driving away, and then untargeted remote sensing on the next. On sol 4493 we start our remote sensing, almost as remote as we can get, with a suprahorizon movie looking for clouds in the south. A dust-devil survey rounds out the sol’s environmental observations, and then the geology theme group can get down to the serious business of looking at rocks. For Mastcam this means observing a group of bedrock targets all called “Observatory Trail” (one of which you can see in the middle of the image above), pointing out some interesting veins in “Point Loma,” and casting their gaze out toward “Black Butte” (which I could not think of a fun pun for…). ChemCam has a LIBS observation of “Cholla,” as well as two long-distance observations of the Texoli Butte and the boxwork structures. Our second sol is a little more restrained, as untargeted sols tend to be. But Curiosity will still have plenty of energy after a good rest. We’re taking advantage of that with an extra-long dust-devil movie. Even though we’re in our cloudy season, we still sometimes see dust lifting, and having that extra time to look out for it increases our chances of catching a wind gust or a dust devil in action. Alongside that we also have a Mastcam tau observation to keep an eye on the amount of dust in the atmosphere, and wrap up with a ChemCam AEGIS activity to autonomously choose a LIBS target.
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Last Updated Mar 28, 2025 Related Terms
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Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions 3 min read
Sols 4447–4449: Looking Back at the Marker Band Valley
NASA’s Mars rover Curiosity captured this image of its workspace using the rover’s Rear Hazard Avoidance Camera (Rear Hazcam) on sol 4447 — or Martian day 4,447 of the Mars Science Laboratory mission — on Feb. 8, 2025, at 13:54:13 UTC. NASA/JPL-Caltech Earth planning date: Friday, Feb. 7, 2025
We are continuing our merry way alongside “Texoli” butte, heading toward the boxworks feature in the distance, our next major waypoint. This is a series of large-scale ridges, which appear from orbital data to be a complex fracture network.
Of course, we don’t actually expect to get there until late fall 2025, at the earliest. Our drives are long right now (the weekend plan has a 50-meter drive, or about 164 feet) but we are still taking the time to document all of the wonderful geology as we go, and not just speeding past all of the cool things!
As Conor mentioned in Wednesday’s blog, power is becoming a challenge right now. Those of us in the northern hemisphere might be thinking (eagerly anticipating!) about the return of Spring but Mars is heading into colder weather, meaning we need to use more power for warming up the rover. However, we are also in a very interesting cloud season (as Conor mentioned), so the environmental theme group (ENV) are keen to do lots of imaging right now. This means very careful planning and negotiating between ENV and the geology theme group (GEO) to make the most of the power we do have. Luckily, this plan has something for everyone.
The GEO group was handed a weekend workspace containing a jumble of rocks — some layered, some not. None of the rocks were very large but we were able to plan APXS and MAHLI on a brushed rock surface at “Aliso Canyon” and on a small, flat unbrushed target, “Bridge to Nowhere,” close to the rover. ChemCam will use the LIBS laser to shoot three bedrock targets, sampling regular bedrock at “Newcomb,” some cracked bedrock at “Devore” and some of the more layered material at “Rubio Canyon.” Mastcam will document the ChemCam LIBS targets. In addition to the cloud imaging, we have lots of other imaging in this plan. We are in position right now to look back down at the “Marker Band Valley,” which we first entered almost a thousand sols ago! Before we go too much further along the side of Texoli butte and lose sight of the Marker Band Valley for some time, both ChemCam and Mastcam will take advantage of this to image the Marker Band Valley and the “Marker Band.” Other images include ChemCam remote images of cap rocks in the distance and two Mastcams of near-field (i.e., close to the rover) troughs.
Written by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick
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Last Updated Feb 10, 2025 Related Terms
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