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By NASA
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 4477-4478: Bumping Back to Business
NASA’s Mars rover Curiosity acquired this image using its Right Navigation Camera on March 10, 2025 — sol 4476, or Martian day 4,476 of the Mars Science Laboratory mission — at 04:15:44 UTC. NASA/JPL-Caltech Written by Sharon Wilson Purdy, Planetary Geologist at the Smithsonian National Air and Space Museum
Earth planning date: Monday, March 10, 2025
The Curiosity rover is winding between the spectacular Gould mesa and Texoli butte through beautifully layered terrain. The end-of-drive target from last week’s plan was a rock with a knobby/bumpy texture that appears quite different from the typical surrounding bedrock. While this interesting rock was in our workspace today, we ended up being just a touch too close to do contact science. As a result, the science team decided to “bump back” (e.g., drive backwards) to get the rover in an ideal position to analyze and characterize this rock on Wednesday.
In the middle of the rover’s workspace today there was a large patch of soil and sand that MAHLI and APXS teamed up to analyze at a target named “Angeles Crest.” Nearby, Mastcam imaged troughs (depressions) along the axis of the sand ridge to understand how they formed. Mastcam had several other targets in the plan that imaged the workspace and surroundings including “Potrero John,” the knobby rock in the workspace, a rock with similar nodular textures in the distance named “Modjeska Peak,” and a light tan rock with a dome-like structure in the vicinity of “Humber Park.”
ChemCam selected a slab of bedrock and loose (“float”) rock in the workspace to characterize their geochemistry with the LIBS instrument at “Millard Canyon” and “Cajon Pass,” respectively. Off in the distance, the science team selected the face of Gould mesa and upper Texoli butte for ChemCam long distance RMI imaging to get a closer look at the rocks, fractures, and layering.
The environmental theme group scheduled several activities to look at clouds, document the atmospheric opacity, and measure the optical depth of the atmosphere and constrain aerosol scattering properties. We have lots of exciting data in hand and more on the road ahead!
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Last Updated Mar 12, 2025 Related Terms
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Mars
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By NASA
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 3 min read
Sols 4475-4476: Even the Best-Laid Plans
NASA’s Mars rover Curiosity acquired this image of “Gould Mesa,” named for a hill near NASA’s Jet Propulsion Laboratory in Southern California, using its Right Navigation Camera on March 6, 2025 — sol 4472, or Martian day 4,472 of the Mars Science Laboratory mission — at 01:37:17 UTC. NASA/JPL-Caltech Written by Deborah Padgett, OPGS Task Lead at NASA’s Jet Propulsion Laboratory
Earth planning date: Friday, March 7, 2025
In Curiosity’s last plan, the team decided to drive toward a very interesting nodular rock. The rover team hoped to do a detailed study of its surface texture over the weekend. However, Curiosity did not receive its expected Friday morning downlink of images taken after its drive. The MSL team did receive a tiny bit of data confirming that Curiosity’s drive finished as expected. Unfortunately, without images to determine exactly where Curiosity was located relative to its intended destination, the team was unable to do any instrument pointing at nearby objects, known as “targeted” observations. However, the rover team showed its resilience by filling the weekend plan with a full slate of fascinating remote observations of the terrain and sky around Curiosity’s current perch, high in the canyons of Mount Sharp. Our science and instrument teams always keep a list of backup observations close at hand — frequently those taking too much time to fit in a typical sol plan — in case they get an unexpected opportunity to use them!
On sol 4475, Curiosity will start its first science block midday with two back-to-back dust-devil surveys with Navcam. These searches for Martian whirlwinds will be followed by a measurement of atmospheric dust with Mastcam. Mastcam will then do its first large panorama image of the plan, an 11×3 mosaic starboard of the rover to document bedrock and regolith in an area with a dark band of material seen from orbit. This long observation will be followed by an AEGIS activity, using Navcam to find targets for ChemCam’s laser spectrograph. Curiosity will then repeat its post-drive imaging at high quality, hopefully to be received at JPL before Monday’s planning day. In the evening, APXS will do atmospheric composition studies for several hours.
The next day will be a “soliday,” without any observations. Early in the morning of sol 4476, Mastcam will take its second large panorama, which will be a fantastic 37×4 mosaic of sunrise on the slopes of Gould Mesa (see image). In the afternoon, there will be a Mastcam dust measurement, ChemCam calibration observation, ChemCam passive sky, and two more dust-devil surveys. The next morning, there will be a set of Navcam cloud movies, a dust measurement, and sky phase function observations to support the Mars aphelion cloud-belt campaign. On sol 4477, we will use the post-drive imaging taken over the weekend to plan contact science, then drive away from this location on sol 4478, continuing Curiosity’s journey toward the mysterious boxwork features to the west.
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Details
Last Updated Mar 11, 2025 Related Terms
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By European Space Agency
Help us uncover the secrets of the Sun! Our Solar Orbiter spacecraft has been watching the Sun since February 2020. With five years’ worth of data waiting to be explored, it’s time to dig in. The new ‘Solar Radio Burst Tracker’ Zooniverse project is ready for you.
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By USH
EBANI stands for "Unidentified Anomalous Biological Entity," referring to a mysterious class of airborne phenomena that may be biological rather than mechanical in nature. These entities are often described as elongated, flexible, and tubular, moving through the sky in a serpentine or twisting manner.
They exhibit advanced flight capabilities, including high-speed travel, precise control, and even self-illumination. Some have been observed rendering themselves invisible, raising questions about their energy sources and possible technological origins.
Recent observations have revealed formations of translucent spheres in red, white, and blue, challenging conventional classifications of both biology and aerodynamics.
Some of these entities have a massive structure composed of thousands of clustered spheres. These entities appear to function as an aircraft carrier, releasing these smaller spheres into Earth's atmosphere for an unknown purpose.
While some researchers propose that EBANIs are natural organisms evolving in Earth's upper atmosphere under unfamiliar physical laws, others speculate they may be advanced artificial (eventually biological) constructs, potentially extraterrestrial probes or surveillance devices, given the presence of large structures expelling numerous smaller spheres.
Are they living UFOs, advanced biological organisms that function autonomously within the spheres, without the need for pilots?
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