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I still remember the first time I saw Saturn through a 10 inch telescope when I was ten years old. It looked just like it did in pictures, a pale yellow disk circled by its stunning ring system. What I couldn't see then were Saturn's moons, including the small, icy world of Enceladus that has since become one of the most exciting targets in the search for life beyond Earth. This tiny moon shoots spectacular plumes of water from cracks in its frozen surface, plumes that contain organic molecules. But a new study suggests we shouldn’t get too excited about what these molecules actually tell us about the possibility of life.

A binary star that has puzzled astronomers for decades may finally be explained. The accretor star is sucking material from its donor star so rapidly that it can't contain it all and is forming a bright, circumbinary ring.

It’s really quite reasonable to assume the stars don’t move! Indeed that was the opinion of our ancestors however we now know they are far from stationary. Imagine a star racing through space so fast it could travel from Earth to the Moon in just three minutes. These are known as hypervelocity white dwarfs and they have puzzled astronomers for years. Now, a team of researchers have finally cracked the mystery of how they get launched at such incredible speeds.

When an interstellar object (ISO) travels through our inner Solar System, the immediate question is "Where did it come from?" There are only fleeing opportunities to study these, since their trajectories take them out of the Solar System pretty quickly. A new research effort aims to understand where the most recent ISO, 3I/ATLAS, originated.

NASA Says Mars Rover Discovered Potential Biosignature Last Year - https://www.nasa.gov/news-release/nasa-says-mars-rover-discovered-potential-biosignature-last-year/ Redox-driven mineral and organic associations in Jezero Crater, Mars - https://www.nature.com/articles/s41586-025-09413-0

Are we alone in the universe? It’s a question that has, despite extensive and sometimes ingenious attempts, yet to be answered. In one of the most ambitious searches for extraterrestrial intelligence ever conducted, Chinese scientists have used the world's largest radio telescope to scan the famous TRAPPIST-1 star system for signs of alien technology. The Five hundred metre Aperture Spherical Telescope is the world's largest single dish radio telescope, and the search for extraterrestrial intelligence (SETI) is one of its five key science objectives.

Science advances through data that don’t fit our current understanding. At least that was Thomas Kuhn’s theory in his famous On the Structure of Scientific Revolutions. So scientists should welcome new data that challenges their understanding of how the universe works. A recent paper, available in pre-print on arXiv, using data from the James Webb Space Telescope (JWST) might just have found some data that can do that. It looked at an exoplanet around a millisecond pulsar and found its atmosphere is made up of almost entirely pure carbon.

Traditionally, black holes are usually thought to reside at the centers of galaxies. However, a research team led by Dr. An Tao from the Shanghai Astronomical Observatory of the Chinese Academy of Sciences has discovered a wandering black hole in a dwarf galaxy located about 230 million light-years away.

It was a chilly night when I peered through my 10” Meade LX200 telescope from Norfolk in the UK! I wasn’t completely convinced it would appear nor even be visible but bang on the prediction, asteroid 2002 MN drifted by my field of view and I was amazed at how accurately we could predict its path! That precision in tracking asteroid trajectories has become even more critical now that we're actively exploring how we can deflect them. A team of scientists have made a discovery about asteroid deflection that's both fascinating and sobering at the same time. Hit an asteroid in the wrong spot, and you might accidentally steer it through a "gravitational keyhole" that sending it back toward Earth years later.

There are plenty of labs working on solutions to Kessler Syndrome, where there’s so much debris in low Earth orbit that rockets are no longer capable of reaching it without being hit with hypersonic parts of defunct equipment. While we haven’t yet gotten to the point where we’ve lost access to space, there will come a day where that will happen if we don’t do something about it. A new paper from Kazunori Takahashi of Tohoku University in Japan looks at a novel solution that uses a type of magnetic field typically seen in fusion reactors to decelerate debris using a plasma beam while balancing itself with an equal and opposite thrust on the other side.

As someone who has lectured for more years than I care to remember and written books about space, I've grown accustomed to constantly rewriting sections as new discoveries emerge. The discovery of the dwarf planet Makemake led to such rewrites, but until now we didn't know much about this elusive world. A team of scientists at the Southwest Research Institute has recently changed that with their detection of methane gas on Makemake using the James Webb Space Telescope. It's exactly the kind of discovery that sends authors like me back to the drawing board, because this finding doesn't just add another detail to Makemake's story, it fundamentally changes how we view these distant worlds.

Interstellar comets are rare, and astronomers don't like to miss an opportunity to observe one. Now the Gemini South Telescope has taken a turn at imaging Comet 3I/ATLAS, the visitor from another star system. The images help show that the comet's tail is growing as it approaches the Sun.

A team of Japanese astronomers has detected protostellar outflow jets in the outer regions of the Milky Way. This is the first detection of this type of jets in this part of the galaxy. Since this part of the galaxy is similar to the more ancient Universe, it's evidence that star formation in the modern Universe is similar to star formation in the ancient Universe.

A new preprint field study reveals that New York City’s rats aren’t just survivors—they’re talkative city dwellers with their own hidden nightlife. Mapping their movements and conversations could offer insights to transform urban planning and pest control

How much of planet Earth is made of water?

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Curiosity Blog, Sols 4649-4654: Ridges, Hollows and Nodules, Oh My NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera, showing the transition from smoother ridge bedrock (right) to more nodular bedrock (bottom left to top middle) on the edge of a shallow hollow (top left). Curiosity, whose masthead shadow is also visible, captured this image on Sept. 5, 2025 — Sol 4650, or Martian day 4,650 of the Mars Science Laboratory mission — at 00:22:34 UTC. NASA/JPL-Caltech

Written by Lucy Thompson, Planetary Scientist and APXS Team Member, University of New Brunswick, Canada

Earth planning date: Friday, Sept. 5, 2025

Curiosity is in the midst of the boxwork campaign, trying to decipher why we see such pronounced ridges and hollows in this area of Mount Sharp. When this terrain was first identified from orbit it was hypothesized that the ridges may be the result of cementation by circulating fluids, followed by differential erosion of the less resistant bedrock in between (the hollows that we now observe). 

We have been exploring the boxwork terrain documenting textures, structures and composition to investigate potential differences between ridges and hollows. One of the textural features we have observed are nodules in varying abundance. The focus of our activities this week was to document the transition from smoother bedrock atop a boxwork ridge to more nodular bedrock associated with the edge of a shallow hollow. 

In Tuesday’s three-sol plan we analyzed the smoother bedrock within the ridge, documenting textures with MAHLI, Mastcam, and ChemCam RMI, and chemistry with ChemCam LIBS and APXS. Curiosity then successfully bumped towards the edge of the ridge/hollow to place the more nodular bedrock in our workspace. Friday’s three-sol plan was basically a repeat of the previous observations, but this time focused on the more nodular bedrock. The planned drive should take us to another boxwork ridge, and closer to the area where we plan to drill into one of the ridges.

As the APXS strategic planner this week, I helped to select the rock targets for analysis by our instrument, ensuring they were safe to touch and that they met the science intent of the boxwork campaign. I also communicated to the rest of the team the most recent results from our APXS compositional analyses and how they fit into our investigation of the boxwork terrain. This will help to inform our fast-approaching decision about where to drill.

Both plans included Mastcam and ChemCam long-distance RMI imaging of more distant features, including other boxwork ridges and hollows, buttes, the yardang unit, and Gale crater rim. Planned environmental activities continue to monitor dust in the atmosphere, dust-devil activity, and clouds. Standard REMS, RAD, and DAN activities round out the week’s activities.

• Want to read more posts from the Curiosity team?

  
  
  Visit Mission Updates
  
  

• Want to learn more about Curiosity’s science instruments?

  
  
  Visit the Science Instruments page
  
  

NASA’s Mars rover Curiosity at the base of Mount Sharp NASA/JPL-Caltech/MSSS

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2 min read

Curiosity Blog, Sols 4649-4654: Ridges, Hollows and Nodules, Oh My NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera, showing the transition from smoother ridge bedrock (right) to more nodular bedrock (bottom left to top middle) on the edge of a shallow hollow (top left). Curiosity, whose masthead shadow is also visible, captured this image on Sept. 5, 2025 — Sol 4650, or Martian day 4,650 of the Mars Science Laboratory mission — at 00:22:34 UTC. NASA/JPL-Caltech

Written by Lucy Thompson, Planetary Scientist and APXS Team Member, University of New Brunswick, Canada

Earth planning date: Friday, Sept. 5, 2025

Curiosity is in the midst of the boxwork campaign, trying to decipher why we see such pronounced ridges and hollows in this area of Mount Sharp. When this terrain was first identified from orbit it was hypothesized that the ridges may be the result of cementation by circulating fluids, followed by differential erosion of the less resistant bedrock in between (the hollows that we now observe). 

We have been exploring the boxwork terrain documenting textures, structures and composition to investigate potential differences between ridges and hollows. One of the textural features we have observed are nodules in varying abundance. The focus of our activities this week was to document the transition from smoother bedrock atop a boxwork ridge to more nodular bedrock associated with the edge of a shallow hollow. 

In Tuesday’s three-sol plan we analyzed the smoother bedrock within the ridge, documenting textures with MAHLI, Mastcam, and ChemCam RMI, and chemistry with ChemCam LIBS and APXS. Curiosity then successfully bumped towards the edge of the ridge/hollow to place the more nodular bedrock in our workspace. Friday’s three-sol plan was basically a repeat of the previous observations, but this time focused on the more nodular bedrock. The planned drive should take us to another boxwork ridge, and closer to the area where we plan to drill into one of the ridges.

As the APXS strategic planner this week, I helped to select the rock targets for analysis by our instrument, ensuring they were safe to touch and that they met the science intent of the boxwork campaign. I also communicated to the rest of the team the most recent results from our APXS compositional analyses and how they fit into our investigation of the boxwork terrain. This will help to inform our fast-approaching decision about where to drill.

Both plans included Mastcam and ChemCam long-distance RMI imaging of more distant features, including other boxwork ridges and hollows, buttes, the yardang unit, and Gale crater rim. Planned environmental activities continue to monitor dust in the atmosphere, dust-devil activity, and clouds. Standard REMS, RAD, and DAN activities round out the week’s activities.

• Want to read more posts from the Curiosity team?

  
  
  Visit Mission Updates
  
  

• Want to learn more about Curiosity’s science instruments?

  
  
  Visit the Science Instruments page
  
  

NASA’s Mars rover Curiosity at the base of Mount Sharp NASA/JPL-Caltech/MSSS

Share

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• 
  
  
• 
  
  
• 
  
  

Details

Last Updated

Sep 12, 2025

Related Terms

• Blogs

Explore More

2 min read Perseverance Meets the Megabreccia

Article


4 days ago

4 min read Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’

Article


1 week ago

2 min read Over Soroya Ridge & Onward!

Article


2 weeks ago

Keep Exploring Discover More Topics From NASA

Mars

Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited…

All Mars Resources

Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,…

Rover Basics

Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a…

Mars Exploration: Science Goals

The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four…

Credit: NASA

NASA has selected Troy Sierra JV, LLC of Huntsville, Alabama, to provide engineering, research, and scientific support at the agency’s Glenn Research Center in Cleveland.  

The Test Facility Operations, Maintenance, and Engineering Services III contract is a cost-plus-fixed-fee, indefinite-delivery/indefinite-quantity contract with a maximum potential value of approximately $388.3 million. The performance period begins Jan. 1, 2026, with a three-year base period followed by a two-year option, and a potential six-month extension through June 2031.

This contract will provide and manage the engineering, technical, manufacturing, development, operations, maintenance, inspection, and certification support services needed to conduct aerospace testing in NASA Glenn’s facilities and laboratories.

For information about NASA and other agency programs, visit:

https://www.nasa.gov

-end-

Tiernan Doyle
Headquarters, Washington
202-358-1600
tiernan.doyle@nasa.gov

Jan Wittry
Glenn Research Center, Cleveland
216-433-5466
jan.m.wittry-1@nasa.gov

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Details Last Updated Sep 12, 2025 LocationNASA Headquarters Related Terms

• Glenn Research Center