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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 The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 2 min read
      Sols 4439-4440: A Lunar New Year on Mars
      NASA’s Mars rover Curiosity captured this image, which includes the prominent wedge-shaped block in the foreground, the imaging target dubbed “Vasquez Rocks” — named after a site in Southern California that’s been a popular filming location for movies and television, including several episodes of “Star Trek.” Curiosity acquired this image using its Left Navigation Camera on sol 4437 — Martian day 4,437 of the Mars Science Laboratory mission — on Jan. 29, 2025, at 04:25:25 UTC. NASA/JPL-Caltech Earth planning date: Wednesday, Jan. 29, 2025
      We’re planning sols 4439 and 4440 on the first day of the Lunar New Year here on Earth, and I’m the Geology/Mineralogy Science Theme Lead for today. The new year is a time for all kinds of abundance and good luck, and we are certainly lucky to be celebrating another new year on Mars with the Curiosity rover!
      The rover’s current position is on the north side of the “Texoli” butte west of the “Rustic Canyon” crater, and we are on our way southwest through the layered sulfate unit toward a possible boxwork structure that we hope to study later this year. Today’s workspace included a couple of representative bedrock blocks with contrasting textures, so we planned an APXS elemental chemistry measurement on one (“Deer Springs”) and a LIBS elemental measurement on another (“Taco Peak”).
      For imaging, there were quite a few targets in view making it possible to advance a variety of science goals. The ChemCam remote imager was used for a mosaic on “Wilkerson Butte” to observe the pattern of resistant and recessive layering. Mastcam mosaics explored some distant landforms (“Sandstone Peak,” “Wella’s Peak”) as well as fractures, block shapes and textures, and aeolian ripples closer to the rover (“Tahquitz Peak,” “Mount Islip,” “Vasquez Rocks,” “Dawson Saddle”). Our regular environmental science measurements were made as well, to track atmospheric opacity and dust activity. So our planning sols include an abundance of targets indeed.
      Fun fact: Today’s name “Vasquez Rocks” comes from a site on Earth in Southern California that has been a popular spot for science fiction filming, appearing in several episodes of “Star Trek” going back to the original series!
      Written by Lucy Lim, Participating Scientist at Goddard Space Flight Center
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      Last Updated Jan 31, 2025 Related Terms
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    • By NASA
      NASA/JPL-Caltech/University of Arizona This Oct. 29, 2018, image from the HiRISE camera on NASA’s Mars Reconnaissance Orbiter captures geysers of gas and dust that occur in springtime in the South Polar region of Mars. As the Sun rises higher in the sky, the thick coating of carbon dioxide ice that accumulated over the winter begins to warm and then turn to vapor. Sunlight penetrates through the transparent ice and is absorbed at the base of the ice layer. The gas that forms because of the warming escapes through weaknesses in the ice and erupts in the form of geysers.
      HiRISE, or the High Resolution Imaging Science Experiment, is a powerful camera that takes pictures covering vast areas of Martian terrain while being able to see features as small as a kitchen table.
      Image credit: NASA/JPL-Caltech/University of Arizona
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    • By NASA
      NASA/Bill Ingalls A NASA photographer captured the full “wolf” moon rising over the Lincoln Memorial and Memorial Bridge on Jan. 13, 2025.
      The Maine Farmers’ Almanac began publishing Native American names for full moons in the 1930s. Over time, these names have become widely known and used. According to this almanac, the full moon in January is called the Wolf Moon, from the packs of wolves heard howling outside the villages amid the cold and deep snows of winter.
      Get tips and guides on skywatching.
      Image credit: NASA/Bill Ingalls
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    • By NASA
      Caption: As part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, Intuitive Machines’ second delivery to the Moon will carry NASA technology demonstrations and science investigations on their Nova-C class lunar lander. Credit: Intuitive Machines For the second time, Intuitive Machines will launch a lunar lander to deliver NASA technology demonstrations and science investigations to the Moon for the benefit of all. Media accreditation is open for the IM-2 launch, part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign to establish a long-term presence on the Moon. 

      The Intuitive Machines Nova-C class lunar lander will launch on a SpaceX Falcon 9 rocket and carry NASA science, technology demonstrations, and other commercial payloads to Mons Mouton, a lunar plateau near the Moon’s South Pole region. Liftoff is targeted for a multi-day launch window, which opens no earlier than late February, from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

      Media prelaunch and launch activities will take place at NASA Kennedy and are open to U.S. citizens and international media. U.S. media must apply by Wednesday, Feb. 12, and international media must apply by Wednesday, Feb. 5.

      Media wishing to take part in person must apply for credentials at:
      https://media.ksc.nasa.gov

      Credentialed media will receive a confirmation email upon approval. NASA’s media accreditation policy is available online. For questions about accreditation or to request special logistical support, such as space for satellite trucks, tents, or electrical connections, please email by Wednesday, Feb. 12, to: ksc-media-accreditat@mail.nasa.gov. For other questions, please contact NASA Kennedy’s newsroom at: 321-867-2468.

      Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo o Messod Bendayan a: antonia.jaramillobotero@nasa.gov o messod.c.bendayan@nasa.gov.

      Among the items on its lander, the IM-2 mission will deliver one of the first on-site, or in-situ, demonstrations of resource utilization on the Moon, using a drill and mass spectrometer to measure the volatiles content of subsurface materials. Other technology instruments on this delivery will demonstrate a robust surface communications system and deploy a propulsive drone mobility solution.

      Launching as a rideshare alongside the IM-2 delivery NASA’s Lunar Trailblazer spacecraft also will begin its journey to lunar orbit, where it will map the distribution of the different forms of water on the Moon.

      A successful landing will help support the CLPS model for commercial payload deliveries to the lunar surface, as another step toward a sustainable lunar future. As a primary customer of CLPS, NASA is investing in lower-cost methods of Moon deliveries and is one of multiple customers for these flights.

      NASA is working with several U.S. companies to deliver science and technology to the lunar surface through the agency’s CLPS initiative. This pool of companies may bid on task orders to deliver NASA payloads to the Moon. Contract awards cover end-to-end commercial payload delivery services, including payload integration, mission operations, launch from Earth, and landing on the surface of the Moon. These contracts are indefinite-delivery/indefinite-quantity contracts with a cumulative maximum value of $2.6 billion through 2028.

      For more information about the agency’s Commercial Lunar Payload Services initiative, see:
      https://www.nasa.gov/clps
      -end-

      Alise Fisher / Jasmine Hopkins
      Headquarters, Washington
      202-358-1600
      alise.m.fisher@nasa.gov / jasmine.s.hopkins@nasa.gov

      Natalia Riusech / Nilufar Ramji
      Johnson Space Center, Houston
      281-483-5111
      natalia.s.riusech@nasa.gov / nilufar.ramji@nasa.gov  

      Antonia Jaramillo
      Kennedy Space Center, Florida
      321-867-2468
      antonia.jaramillobotero@nasa.gov
      Share
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      Last Updated Jan 24, 2025 LocationJohnson Space Center Related Terms
      Missions Artemis Commercial Lunar Payload Services (CLPS) View the full article
    • By NASA
      4 Min Read NASA Space Tech’s Favorite Place to Travel in 2025: The Moon!
      The first image from space of Firefly's Blue Ghost mission 1 lunar lander as it begins its 45-day transit period to the Moon. Credits: Firefly Aerospace NASA Space Technology has big travel plans for 2025, starting with a trip to the near side of the Moon!
      Among ten groundbreaking NASA science and technology demonstrations, two technologies are on a ride to survey lunar regolith – also known as “Moon dust” – to better understand surface interactions with incoming lander spacecraft and payloads conducting experiments on the surface. These dust demonstrations and the data they’re designed to collect will help support future lunar missions.  
      Blue Ghost Mission 1 launched at 1:11 a.m. EST aboard a SpaceX Falcon 9 rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida. The company is targeting a lunar landing on Sunday, March 2. 
      The first image from space of Firefly’s Blue Ghost mission 1 lunar lander as it begins its 45-day transit period to the Moon. Firefly Aerospace NASA Space Technology on Blue Ghost Mission 1
      NASA’s Electrodynamic Dust Shield (EDS) will lift, transport, and remove particles using electric fields to repel and prevent hazardous lunar dust accumulation on surfaces. The agency’s Stereo Camera for Lunar Plume-Surface Studies (SCALPSS) technology will use stereo imaging to capture the impact of rocket plumes on lunar regolith as the lander descends to the Moon’s surface, returning high-resolution images that will help in creating models to predict regolith erosion – an important task as bigger, heavier payloads are delivered to the Moon in close proximity to each other. 
      The EDS and SCALPSS technologies will be delivered to the Moon on Firefly’s first Blue Ghost mission, named Ghost Riders in the Sky, as part of NASA’s CLPS (Commercial Lunar Payload Services) initiative. Its landing target is a 300-mile-wide basin located on the Moon’s near side, called Mare Crisium – a large, dark, basaltic plain that filled an ancient asteroid impact. First-of-their-kind experiments will deploy after landing to gather important data in a broad spectrum of areas including geophysical characteristics, global navigation, radiation tolerant computing, and the behavior of lunar regolith.
      Replicating the Moon’s harsh environment on Earth is a significant challenge because of extreme temperatures, low gravity, radiation, and dusty surface. The CLPS initiative provides unprecedented access to the lunar surface, allowing us to demonstrate technologies in the exact conditions they were designed for. Missions like Blue Ghost Mission 1 are a true game changer for NASA technology advancement and demonstration.”
      Michael Johansen
      Flight Demonstrations Lead for NASA’s Game Changing Development program
      Dust particles scatter during an experiment for the Electrodynamic Dust Shield in a laboratory at NASA’s Kennedy Space Center in Florida. NASA NASA’s Stereo Camera for Lunar Plume-Surface Studies technology integrated on Firefly’s Blue Ghost lander. Firefly Aerospace A complex wrinkle ridge in Mare Crisium at low Sun, seen in an image captured by the Lunar Reconnaissance Orbiter Camera.NASA/GSFC/Arizona State University Understanding regolith
      The Moon’s dusty environment was one of the greatest challenges astronauts faced during Apollo Moon missions, posing hazards to lunar surface systems, space suits, habitats, and instrumentation. What was learned from those early missions – and from thousands of experiments conducted on Earth and in space since – is that successful surface missions require the ability to eliminate dust from all kinds of systems. Lunar landings, for example, cause lunar dust to disperse in all directions and collect on everything that lands there with it. This is one of the reasons such technologies are important to understand. The SCALPSS technology will study the dispersion of lunar dust, while EDS will demonstrate a solution to mitigate it. 

      Getting this new data on lunar regolith with be pivotal for our understanding of the lunar surface. We’ve long known that lunar dust is a huge challenge. The Lunar Surface Innovation Initiative has enabled us to initiate lunar dust mitigation efforts across the agency, working with industry and international partners. The lunar science, exploration, and technology communities are eager to have new quantitative data, and to prove laboratory experiments and develop technology solutions.”
      Kristen John
      Technical Integration Lead for NASA’s Lunar Surface Innovation Initiative (LSII)
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      [VIDEO] Dust on the lunar surface is a significant hazard for systems and astronauts living and working on the Moon. NASA space technologies are developing solutions to retire hurdles in this capability area. NASA Space Technology Dust mitigation technology has come a long way, but we still have a lot to learn to develop surface systems and infrastructure for more complex missions. LSII is actively engaged in this effort, working with the lunar community across sectors to expand knowledge and design new approaches for future technologies. Working alongside the Lunar Surface Innovation Consortium, LSII has a unique opportunity to take a holistic look at dust’s role in the development of surface infrastructure with other key capability areas including in-situ resource utilization, surface power, and surviving the lunar night.  
      Learning from the the Moon benefits Mars science and exploration
      Capabilities for minimizing dust interaction are as important for future missions on Mars as it is for missions on the Moon. Like the Moon, Mars is also covered with regolith, also called Martian dust or Martian soil, but the properties are different than lunar regolith, both in shape and mineralogy. The challenges Mars rovers have encountered with Martian regolith have provided great insight into the challenges we will face during lunar surface missions. Learning is interwoven and beneficial to future missions whether hundreds of thousands of miles from Earth, on the Moon, or millions, on Mars.  

      Scientist-astronaut Harrison Schmitt, Apollo 17 lunar module pilot, uses an adjustable sampling scoop to retrieve lunar samples during the second Apollo 17 extravehicular activity (EVA). NASA NASA’s Perseverance Mars rover snagged two samples of regolith – broken rock and dust – on Dec. 2 and 6, 2022. This set of images, taken by the rover’s left navigation camera, shows Perseverance’s robotic arm over the two holes left after the samples were collected.NASA/JPL-Caltech Learn more from a planetary scientist about how science factors into lunar dust mitigation technologies:
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      Last Updated Jan 24, 2025 LocationNASA Headquarters Related Terms
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