Sols 4229-4231: More Analyses of the Mammoth Lakes 2 Sample!

Sols 4229-4231: More Analyses of the Mammoth Lakes 2 Sample!

2 min read

Sols 4229-4231: More Analyses of the Mammoth Lakes 2 Sample!

A black and white photograph of
The inlet into to the SAM instrument open and awaiting sample delivery. This image was taken by Right Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4226 (2024-06-26 11:06:46 UTC).

Earth Planning Date: Friday, June 28, 2024

After reviewing results from the Evolved Gas Analysis (EGA) experiment that were downlinked yesterday afternoon (Sols 4226-4228: A Powerful Balancing Act), the SAM team decided they’d like to go ahead with a second experiment to analyze the Mammoth Lakes 2 drilled sample. This experiment is known as the Gas Chromatograph/Mass Spectrometer (GCMS) experiment.

SAM, whose full name is Sample Analysis at Mars, is actually a suite of three different analytical instruments that are used to measure the composition of gases which come off drilled samples as we bake them in SAM’s ovens. The three analytical instruments are called a gas chromatograph, quadrupole mass spectrometer, and tunable laser spectrometer. Each one is particularly suited for measuring specific kinds of compounds in the gases, and these include things like water, methane, carbon, or organic (carbon-containing) molecules. In the EGA experiment that we ran in our last plan, we baked the Mammoth Lakes 2 sample and measured the gas compositions using the tunable laser spectrometer and quadrupole mass spectrometer. In this plan, we’ll deliver a new pinch of sample to the SAM oven and then measure the composition of the gases that are released using the gas chromatograph and quadrupole mass spectrometer. By running both experiments, we’ll have a more thorough understanding of the materials that are in this rock.

The SAM GCMS experiment takes a lot of power to run, so it will be the focus of today’s three-sol plan. However, we still managed to fit in some other science activities around the experiment, including a ChemCam RMI mosaic of some far-off ridges, a ChemCam LIBS observation of a nodular target named “Trail Lakes,” environmental monitoring activities, and a couple Mastcam mosaics to continue imaging the terrain around the rover. Should be another fun weekend of science in Gale crater!

Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory

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NASA’s NEOWISE Infrared Heritage Will Live On

NASA’s NEOWISE Infrared Heritage Will Live On

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA’s near-Earth-object-hunting mission NEOWISE is nearing its conclusion. But its work will carry on with NASA’s next-generation infrared mission: NEO Surveyor.

After more than 14 successful years in space, NASA’s NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer) mission will end on July 31. But while the mission draws to a close, another is taking shape, harnessing experience gained from NEOWISE: NASA’s NEO Surveyor (Near Earth Object Surveyor), the first purpose-built infrared space telescope dedicated to hunting hazardous near-Earth objects. Set for launch in late 2027, it’s a major step forward in the agency’s planetary defense strategy.

“After developing new techniques to find and characterize near-Earth objects hidden in vast quantities of its infrared survey data, NEOWISE has become key in helping us develop and operate NASA’s next-generation infrared space telescope. It is a precursor mission,” said Amy Mainzer, principal investigator of NEOWISE and NEO Surveyor at the University of California, Los Angeles. “NEO Surveyor will seek out the most difficult-to-find asteroids and comets that could cause significant damage to Earth if we don’t find them first.”

WISE mission’s telescope is worked on by engineers
Seen here in a clean room at the Space Dynamics Laboratory in Logan, Utah, the WISE mission’s telescope is worked on by engineers. Avionics hardware and solar panels would later be attached before the spacecraft’s launch on Dec. 14, 2009.
SDL

WISE Beginnings

NEOWISE’s end of mission is tied to the Sun. About every 11 years, our star experiences a cycle of increased activity that peaks during a period called solar maximum. Explosive events, such as solar flares and coronal mass ejections, become more frequent and heat our planet’s atmosphere, causing it to expand. Atmospheric gases, in turn, increase drag on satellites orbiting Earth, slowing them down. With the Sun currently ramping up to predicted maximum levels of activity, and with no propulsion system for NEOWISE to keep itself in orbit, the spacecraft will soon drop too low to be usable.

The infrared telescope is going out of commission having exceeded scientific objectives for not one, but two missions, beginning as WISE (Wide-field Infrared Survey Explorer).

Managed by NASA’s Jet Propulsion Laboratory in Southern California, WISE launched in December 2009 with a six-month missionto scan the entire infrared sky. By July 2010, WISE had achieved this with far greater sensitivity than previous surveys, and NASA extended the mission until 2011.

During this phase, WISE studied distant galaxies, outgassing comets, exploding white dwarf stars, and brown dwarfs. It identified tens of millions of actively feeding supermassive black holes. It also generated data on circumstellar disks — clouds of gas, dust, and rubble spinning around stars — that citizen scientists continue to mine through the Disk Detective project.

In addition, it excelled at finding main belt asteroids, as well as near-Earth objects, and discovered the first known Earth Trojan asteroid. What’s more, the mission provided a census of dark, faint near-Earth objects that are difficult for ground-based telescopes to detect, revealing that these objects constitute a sizeable fraction of the near-Earth object population.

Comet NEOWISE was discovered by its namesake mission on March 27, 2020, and became a dazzling celestial object visible in the Northern Hemisphere for several weeks that year. It was one of 25 comets discovered by the mission.
SDL/Allison Bills

Infrared Heritage

Invisible to the naked eye, infrared wavelengths are emitted by warm objects. To keep the heat generated by WISE itself from interfering with its infrared observations, the spacecraft relied on cryogenic coolant. By the time the coolant had run out, WISE had mapped the sky twice, and NASA put the spacecraft into hibernation in February 2011.

Soon after, Mainzer and her team proposed a new mission for the spacecraft: to search for, track, and characterize near-Earth objects that generate a strong infrared signal from their heating by the Sun.

“Without coolant, we had to find a way to cool the spacecraft down enough to measure infrared signals from asteroids,” said Joseph Masiero, NEOWISE deputy principal investigator and a scientist at IPAC, a research organization at Caltech in Pasadena, California. “By commanding the telescope to stare into deep space for several months, we determined it would radiate only enough heat to reach lower temperatures that would still allow us to acquire high-quality data.” NASA reactivated the mission in 2013 under the Near-Earth Object Observations Program, a precursor to the agency’s current planetary defense program, with the new name NEOWISE.

By repeatedly observing the sky from low Earth orbit, NEOWISE has made 1.45 million infrared measurements of over 44,000 solar system objects to date. That includes more than 3,000 NEOs, 215 of which the space telescope discovered. Twenty-five of those are comets, among them the famed comet NEOWISE that was visible in the night sky in the summer of 2020.

“The spacecraft has surpassed all expectations and provided vast amounts of data that the science community will use for decades to come,” said Joseph Hunt, NEOWISE project manager at JPL. “Scientists and engineers who worked on WISE and through NEOWISE also have built a knowledge base that will help inform future infrared survey missions.”

The space telescope will continue its survey until July 31. Then, on Aug. 8, mission controllers at JPL will send a command that puts NEOWISE into hibernation for the last time. Since its launch, NEOWISE’s orbit has been dropping closer to Earth. NEOWISE is expected to burn up in our planet’s atmosphere sometime between late 2024 and early 2025.

More About the Mission

NEOWISE and NEO Surveyor support the objectives of NASA’s Planetary Defense Coordination Office (PDCO) at NASA Headquarters in Washington. The NASA Authorization Act of 2005 directed NASA to discover and characterize at least 90% of the near-Earth objects more than 140 meters (460 feet) across that come within 30 million miles (48 million kilometers) of our planet’s orbit. Objects of this size can cause significant regional damage, or worse, should they impact the Earth.

JPL manages and operates the NEOWISE mission for PDCO within the Science Mission Directorate. The Space Dynamics Laboratory in Logan, Utah, built the science instrument. Ball Aerospace & Technologies Corp. of Boulder, Colorado, built the spacecraft. Science data processing, archiving, and distribution is done at IPAC at Caltech. Caltech manages JPL for NASA.

For more information about NEOWISE, visit:

https://www.nasa.gov/neowise

Media Contacts

Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov

Karen Fox / Charles Blue
NASA Headquarters, Washington
202-358-1600 / 202-802-5345
karen.c.fox@nasa.gov / charles.e.blue@nasa.gov

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Anthony Greicius

Cassini Sees Saturn

Cassini Sees Saturn

Saturn and its rings against the blackness of space. Saturn is a pale beige, with slightly varying stripes. At the top is a sliver of blue light.
NASA/JPL/Space Science Institute

The Cassini-Huygens spacecraft captured this last “eyeful” of Saturn and its rings on March 27, 2004, as it continued its way to orbit insertion. This natural color image shows the color variations between atmospheric bands and features in the southern hemisphere of Saturn, subtle color differences across the planet’s middle B ring, as well as a bright blue sliver of light in the northern hemisphere – sunlight passing through the Cassini Division in Saturn’s rings and being scattered by the cloud-free upper atmosphere.

Cassini-Huygens, at 12,593 pounds one of the heaviest planetary probes ever, was launched on Oct. 15, 1997, on a Titan IVB/Centaur rocket from Cape Canaveral Air Force Station in Florida. Although that was the most powerful expendable launch vehicle available, it wasn’t powerful enough to send the massive Cassini-Huygens on a direct path to Saturn. Instead, the spacecraft relied on several gravity assist maneuvers to achieve the required velocity to reach the ringed planet. This seven-year journey took it past Venus twice, the Earth once, and Jupiter once, gaining more velocity with each flyby for the final trip to Saturn.

On July 1, 2004, with the Huygens lander still attached, Cassini fired its main engine for 96 minutes and entered an elliptical orbit around Saturn, becoming the first spacecraft to do so. Thus began an incredible 13-year in-depth exploration of the planet, its rings and its satellites, with scores of remarkable discoveries.

The Cassini mission ended on Saturn in 2015, when operators deliberately plunged the spacecraft into the planet to ensure Saturn’s moons remain pristine for future exploration.

Image Credit: NASA/JPL/Space Science Institute

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Monika Luabeya

NASA’s Upgraded Hyperwall Offers Improved Data Visualization

NASA’s Upgraded Hyperwall Offers Improved Data Visualization

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NAS visualization & data sciences lead Chris Henze demonstrates the newly upgraded hyperwall visualization system to Ames center director Eugene Tu, deputy center director David Korsmeyer, and High-End Computing Capability manager William Thigpen.
NASA/Brandon Torres Navarette

In May, the NASA Advanced Supercomputing (NAS) facility, located at NASA’s Ames Research Center in California’s Silicon Valley, celebrated the newest generation of its hyperwall system, a wall of LCD screens that display supercomputer-scale visualizations of the very large datasets produced by NASA supercomputers and instruments. 

The upgrade is the fourth generation of hyperwall clusters at NAS. The LCD panels provide four times the resolution of the previous system, now spanning across a 300-square foot display with over a billion pixels. The hyperwall is one of the largest and most powerful visualization systems in the world. 

Systems like the NAS hyperwall can help researchers visualize their data at large scale, across different viewpoints or using different parameters for new ways of analysis. The improved resolution of the new system will help researchers “zoom in” with greater detail. 

The hyperwall is just one way researchers can utilize NASA’s high-end computing technology to better understand their data. The NAS facility offers world-class supercomputing resources and services customized to meet the needs of about 1,500 users from NASA centers, academia and industry. 

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Tara Friesen

NASA Awards Support STEM Research at Minority Serving Institutions

NASA Awards Support STEM Research at Minority Serving Institutions

A photo of MPLAN principal investigator awardees from various minority-serving institutions at the 2023 NASA Better Together conference in San Jose, California.
Credits: NASA

NASA has selected 23 minority-serving institutions to receive $1.2 million to grow their research and technology capabilities, collaborate on research projects, and contribute to the agency’s missions for the benefit of humanity.

Through NASA’s Minority University Research and Education Project (MUREP) Partnership Learning Annual Notification (MPLAN) award, selected institutions will receive up to $50,000 each for a six-month period to work directly on STEM projects with subject matter experts in NASA’s mission directorates.

“As NASA looks to inspire the next generation, the Artemis Generation, we are intentional in increasing access for all,” said Shahra Lambert, NASA senior advisor for engagement and equity. “It’s a daring task to return to the Moon then venture to Mars, but NASA is known to make the impossible possible. By funding partnerships such as MPLAN, and tapping into all pools of STEM resources, including MSIs, we are ensuring the future of our missions are in good hands.”

The awards will contribute to research opportunities in preparation for larger funding programs such as NASA’s annual Small Business Innovation Research/Small Business Technology Transfer solicitation, the Space Technology Research Grant Program within the agency’s Space Technology Mission Directorate, the University Leadership Initiative within the Aeronautics Research Mission Directorate, and the Human Research Program within NASA’s Space Operations Mission Directorate.

“These awards will help unlock the full potential of students traditionally underrepresented in science, technology, engineering, and mathematics research and careers,” said Torry Johnson, deputy associate administrator of STEM Engagement Projects at NASA Headquarters in Washington. “Through this award, universities receive support, resources, and guidance directly from NASA experts, which can be a game changer for the work they do to develop technological innovations that contribute to NASA missions and benefit all of humanity.”

The awardees are as follows:

  • Arizona State University

Drones for Contact-inclusive Planetary Exploration

  • California State University-Dominguez Hills

Bioinspired Surface Design for Thermal Extremes

  • California State University-Fresno

Human-Centric Digital Twins in NASA Space Missions

  • California State University-Northridge

Repurposing Lander Parts into Geodesic Assemblies

  • California State University, Monterey Bay

Crafting Biofuels via Molecular Insights

  • CUNY New York City College of Technology

Polyethylene Glycol Diacrylate for Seed Growth: Microgreens in Space

  • Delgado Community College, New Orleans, Louisiana

Freshmen Access to CubeSat Education

  • Fayetteville State University, Fayetteville, North Carolina

New Tech for Storm Tracking with Machine Learning

  • Hampton University, Hampton, Virginia

Sustained Approach for Energetic Lunar Operation

  • New Mexico Institute of Mining and Technology

Information-Theoretic Multi-Robot Exploration

  • Portland State University, Portland, Oregon

Robot Leg Design for Lunar Exploration

  • Regents of New Mexico State University

Extreme Aerodynamics Over Small Air Vehicles

  • San Diego State University

Enhanced Aero-Composites: Reinforcement Innovation

  • San Francisco State University

Early Non-invasive Diagnosis of Heart Diseases

  • San Jose State University

Designing Resilient Battery System for Space

  • Southern University and A & M College, Baton Rouge, Louisiana

X-Ray 3D Printing of Nanocomposites for AME

Plant Antimicrobial in Space Exploration using AI

  • Spelman College, Atlanta, Georgia

Non-contact Optical Sensor for Biomedicine

  • The Research Foundation of CUNY on behalf of City College, New York

Soft Tendril-inspired Robot for Space Exploration

  • The University of Texas at San Antonio

Hydrodynamic Stability of Jets via Neural Networks

Low-SWaP Water Electrolyzer for Lunar/Martian In-Situ Resource Utilization

  • The University of Texas Rio Grande Valley

Tuneable NanoEnergetic Microthruster Cartridges

  • University of California, Irvine

Flexible Modular Robots for Extreme Access

  • University of Hawaii at Manoa

Ultrasound methods for monitoring carcinogenesis

  • University of New Mexico

All-climate and Ultrafast Aluminum Ion Batteries

The awarded institutions and their partners are invited to meet with NASA researchers and MUREP representatives throughout the remainder of 2024. The meetings serve as training sessions to pursue future NASA opportunities. These trainings focus primarily on fostering collaboration, enhancing technical skills, and providing insights into NASA’s research priorities to better prepare participants for future opportunities.

To learn more about MPLAN, visit:

https://go.nasa.gov/49gsZ9X

-end-

Gerelle Dodson
Headquarters, Washington
202-358-1600
gerelle.q.dodson@nasa.gov

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Tiernan P. Doyle