{"id":788363,"date":"2024-09-04T15:36:50","date_gmt":"2024-09-04T20:36:50","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=788363"},"modified":"2024-09-04T15:36:50","modified_gmt":"2024-09-04T20:36:50","slug":"the-marshall-star-for-september-4-2024","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=788363","title":{"rendered":"The Marshall Star for September 4, 2024"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<p>NASA is making strides with the\u00a0Artemis campaign\u00a0as key components for the SLS (Space Launch System) rocket continue to make their way to\u00a0NASA\u2019s Kennedy Space Center. Teams with NASA and Boeing loaded the core stage boat-tail for Artemis III and the core stage engine section for Artemis IV onto the agency\u2019s Pegasus barge at\u00a0Michoud Assembly Facility\u00a0on Aug. 28.<\/p>\n<p>The core stage hardware joins the launch vehicle stage adapter for Artemis II, which was moved onto the barge at\u00a0NASA\u2019s Marshall Space Flight Center\u00a0on Aug. 21. Pegasus will ferry the multi-mission rocket hardware more than 900 miles to the Space Coast of Florida. Teams with the NASA\u2019s Exploration Ground Systems Program will prepare the launch vehicle stage adapter for Artemis II stacking operations inside the Vehicle Assembly Building, while the core stage hardware will be moved to Kennedy\u2019s Space Systems Processing Facility for outfitting. Beginning with Artemis III, core stages will undergo final assembly\u00a0at Kennedy.<\/p>\n<p>The launch vehicle stage adapter is essential for connecting the rocket\u2019s core stage to the upper stage. It also shields sensitive avionics and electrical components in the rocket\u2019s interim cryogenic propulsion stage from the intense vibrations and noise of launch.<\/p>\n<p>The boat-tail and engine section are crucial for the rocket\u2019s functionality. The boat-tail extends from the engine section, fitting snugly to protect the rocket\u2019s engines during launch. The engine section itself houses more than 500 sensors, 18 miles of cables, and key systems for fuel management and engine control, all packed into the bottom of the towering 212-foot core stage.<\/p>\n<p>NASA is working to land the first woman, first person of color, and its first international partner astronaut on the Moon under Artemis. SLS is part of NASA\u2019s backbone for deep space exploration, along with the Orion spacecraft, supporting ground systems, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single launch.<\/p>\n<p>Marshall manages the SLS Program and Michoud.<\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<p><em>By Wayne Smith<\/em><\/p>\n<p>NASA\u2019s Student Launch competition kicks off its 25th year with the release of the 2025 handbook, detailing how teams can submit proposals by Sept. 11 for the event scheduled next spring near NASA\u2019s Marshall Space Flight Center.<\/p>\n<p>Student Launch is an annual competition challenging middle school, high school, and college students to design, build, test, and launch a high-powered amateur rocket with a scientific or engineering payload. After a team is selected, they must meet documentation milestones and undergo detailed reviews throughout the school year.<\/p>\n<p>Each year, NASA updates the university payload challenge to reflect current scientific and exploration missions. For the 2025 season, the payload challenge will again take inspiration from the\u00a0Artemis\u00a0missions, which seek to land the first woman and first person of color on the\u00a0Moon.<\/p>\n<p>As Student Launch celebrates its 25th anniversary, the payload challenge will include \u201creports\u201d from\u00a0STEMnauts, non-living objects representing astronauts. The 2024 challenge tasked teams with safely deploying a lander mid-air for a group of four STEMnauts using metrics to support a survivable landing. The lander had to be deployed without a parachute and had a minimum weight limit of five pounds.<\/p>\n<p>\u201cThis year, we\u2019re shifting the focus to communications for the payload challenge,\u201d said John Eckhart, technical coordinator for Student Launch at Marshall. \u201cThe STEMnaut \u2018crew\u2019 must relay real-time data to the student team\u2019s mission control. This helps connect Student Launch with the Artemis missions when NASA lands astronauts on the Moon.\u201d<\/p>\n<p>Thousands of students participated in the\u00a02024 Student Launch competition\u00a0\u2013 making up 70 teams representing 24 states and Puerto Rico. Teams launched their rockets to an altitude between 4,000 and 6,000 feet, while attempting to make a successful landing and executing the payload mission. The University of Notre Dame was the overall winner of the 2024 event, which culminated with a launch day open to the public.<\/p>\n<p>Student Launch began in 2000 when former Marshall Director Art Stephenson started a student rocket competition at the center. It started with just two universities in Huntsville competing \u2013 Alabama A&amp;M University and the University of Alabama in Huntsville \u2013 but has continued to soar. Since its inception, thousands of students have participated in the agency\u2019s STEM competition, with many\u00a0going on to a career with NASA.<\/p>\n<p>\u201cThis remarkable journey, spanning a quarter of a century, has been a testament to the dedication, ingenuity, and passion of countless students, educators, and mentors who have contributed to the program\u2019s success,\u201d Eckhart said. \u201cNASA Student Launch has been at the forefront of experiential education, providing students from middle school through university with unparalleled opportunities to engage in real-world engineering and scientific research. The program\u2019s core mission \u2013 to inspire and cultivate the next generation of aerospace professionals and space explorers \u2013 has not only been met but exceeded in ways we could have only dreamed of.\u201d<\/p>\n<p>To encourage students to pursue degrees and careers in STEM (science, technology, engineering, and math), Marshall\u2019s Office of STEM Engagement hosts Student Launch, providing them with real-world experiences. Student Launch is one of NASA\u2019s nine\u00a0Artemis Student Challenges\u00a0\u2013 a variety of activities that expose students to the knowledge and technology required to achieve the goals of Artemis.\u00a0<\/p>\n<p>In addition to the\u00a0NASA Office of STEM Engagement\u2019s\u00a0Next Generation STEM project, NASA Space Operations Mission Directorate, Northrup Grumman, National Space Club Huntsville, American Institute of Aeronautics and Astronautics, National Association of Rocketry, Relativity Space and Bastion Technologies provide funding and leadership for the competition.\u00a0<\/p>\n<p>\u201cThese bright students rise to a nine-month challenge for Student Launch that tests their skills in engineering, design, and teamwork,\u201d said Kevin McGhaw, director of NASA\u2019s Office of STEM Engagement Southeast Region. \u201cThey are the Artemis Generation, the future scientists, engineers, and innovators who will lead us into the future of space exploration.\u201d<\/p>\n<p><em>Smith, a Media Fusion employee and the Marshall Star editor, supports the Marshall Office of Communications.<\/em><\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<p><em>By Wayne Smith<\/em><\/p>\n<p>Following a 2024 competition that garnered international attention, NASA is expanding its\u00a0Human Exploration Rover Challenge\u00a0(HERC) to include a remote control division and inviting middle school students to participate.<\/p>\n<p>The 31st annual competition is scheduled for April 11-12, 2025, at the U.S. Space &amp; Rocket Center, near NASA\u2019s\u00a0Marshall Space Flight Center. HERC is managed by NASA\u2019s Southeast Regional\u00a0Office of STEM Engagement\u00a0at Marshall. The\u00a0HERC 2025 Handbook\u00a0has been released, with guidelines for the new remote control (RC) division \u2013 ROVR (Remote-Operated Vehicular Research) \u2013 and detailing updates for the human-powered division.<\/p>\n<p>\u201cOur RC division significantly lowers the barrier to entry for schools who don\u2019t have access to manufacturing facilities, have less funding, or who are motivated to compete but don\u2019t have the technical mentorship required to design and manufacture a safe human-powered rover,\u201d said Chris Joren, HERC technical coordinator. \u201cWe are also opening up HERC to middle school students for the first time. The RC division is inherently safer and less physically intensive, so we invite middle school teams and organizations to submit a proposal to be a part of HERC 2025.\u201d<\/p>\n<p>Another change for 2025 is the removal of task sites on the course for the human-powered rover division, allowing teams to focus on their rover\u2019s design. Recognized as NASA\u2019s leading international student challenge, the 2025 challenge aims to put competitors in the mindset of the Artemis campaign as they pitch an engineering design for a lunar terrain vehicle \u2013 they are astronauts piloting a vehicle, exploring the lunar surface while overcoming various obstacles.<\/p>\n<p>\u201cThe HERC team wanted to put together a challenge that allows students to gain 21st century skills, workforce readiness skills, and skills that are transferable,\u201d said Vemitra Alexander, HERC activity lead. \u201cThe students have opportunities to learn and apply the engineering design process model, gain public speaking skills, participate in community outreach, and learn the art of collaborating with their peers. I am very excited about HERC\u2019s growth and the impact it has on the students we serve nationally and internationally.\u201d<\/p>\n<p>Students interested in designing, developing, building, and testing rovers for Moon and Mars exploration are invited to submit their proposals to NASA through Sept. 19.<\/p>\n<p>More than 1,000 students with 72 teams from around the world participated in the\u00a02024 challenge\u00a0as HERC celebrated its 30th anniversary as a NASA competition. Participating\u00a0teams\u00a0represented 42 colleges and\u00a0universities and 30 high schools from 24 states, the District of Columbia, Puerto Rico, and 13 other nations from around the world.<\/p>\n<p>\u201cWe saw a massive jump in recognition, not only from within the agency as NASA Chief Technologist A.C. Charania attended the event, but with several of our international teams meeting dignitaries and ambassadors from their home countries to cheer them on,\u201d Joren said. \u201cThe most impressive thing will always be the dedication and resilience of the students and their mentors. No matter what gets thrown at these students, they still roll up to the start line singing songs and waving flags.\u201d<\/p>\n<p>HERC is one of NASA\u2019s eight\u00a0Artemis Student Challenges\u00a0reflecting the goals of the\u00a0Artemis\u00a0campaign, which seeks to land the first woman and first person of color on the Moon while establishing a long-term presence for science and exploration. NASA uses such challenges to encourage students to pursue degrees and careers in the STEM fields of science, technology, engineering, and mathematics.\u00a0<\/p>\n<p>Since its inception in 1994, more than 15,000 students have participated in HERC \u2013 with many\u00a0former students\u00a0now working at NASA, or within the aerospace industry.\u00a0\u00a0\u00a0\u00a0<\/p>\n<p><em>Smith, a Media Fusion employee and the Marshall Star editor, supports the Marshall Office of Communications.<\/em><\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<p>A quarter of a century ago, NASA released the \u201cfirst light\u201d images from the agency\u2019s Chandra X-ray Observatory. This introduction to the world of Chandra\u2019s high-resolution X-ray imaging capabilities included an unprecedented view of Cassiopeia A, the remains of an exploded star located about 11,000 light-years from Earth. Over the years, Chandra\u2019s views of Cassiopeia A have become some of the telescope\u2019s best-known images.<\/p>\n<p>To mark the anniversary of this milestone, new sonifications of three images \u2013 including Cassiopeia A (Cas A) \u2013 are being released. Sonification is a process that translates astronomical data into sound, similar to how digital data are more routinely turned into images. This translation process preserves the science of the data from its original digital state but provides an alternative pathway to experiencing the data.<\/p>\n<p>This sonification of Cas A features data from Chandra as well as NASA\u2019s James Webb, Hubble, and retired Spitzer space telescopes. The scan starts at the neutron star at the center of the remnant, marked by a triangle sound, and moves outward. Astronomers first saw this neutron star when Chandra\u2019s inaugural observations were released 25 years ago this week. Chandra\u2019s X-rays also reveal debris from the exploded star that is expanding outward into space. The brighter parts of the image are conveyed through louder volume and higher pitched sounds. X-ray data from Chandra are mapped to modified piano sounds, while infrared data from Webb and Spitzer, which detect warmed dust embedded in the hot gas, have been assigned to various string and brass instruments. Stars that Hubble detects are played with crotales, or small cymbals.<\/p>\n<p>Another new sonification features the spectacular cosmic vista of 30 Doradus, one of the largest and brightest regions of star formation close to the Milky Way. This sonification again combines X-rays from Chandra with infrared data from Webb. As the scan moves from left to right across the image, the volume heard again corresponds to the brightness seen. Light toward the top of the image is mapped to higher pitched notes. X-rays from Chandra, which reveal gas that has been superheated by shock waves generated by the winds from massive stars, are heard as airy synthesizer sounds. Meanwhile, Webb\u2019s infrared data show cooler gas that provides the raw ingredients for future stars. These data are mapped to a range of sounds including soft, low musical pitches (red regions), a wind-like sound (white regions), piano-like synthesizer notes indicating very bright stars, and a rain-stick sound for stars in a central cluster.<\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube\">\n<p>\n<iframe loading=\"lazy\" title=\"#NASA Sonification of Cassiopeia A\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/X3Oh3DmY2oM?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/p>\n<\/figure>\n<p>The final member of this new sonification triumvirate is NGC 6872, a large spiral galaxy that has two elongated arms stretching to the upper right and lower left, which is seen in an optical light view from Hubble. Just to the upper left of NGC 6872 appears another smaller spiral galaxy. These two galaxies, each of which likely has a supermassive black hole at the center, are being drawn toward one another. As the scan sweeps clockwise from 12 o\u2019clock, the brightness controls the volume and light farther from the center of the image is mapped to higher-pitched notes. Chandra\u2019s X-rays, represented in sound by a wind-like sound, show multimillion-degree gas that permeates the galaxies. Compact X-ray sources from background galaxies create bird-like chirps. In the Hubble data, the core of NGC 6872 is heard as a dark low drone, and the blue spiral arms (indicating active star formation) are audible as brighter, more highly pitched tones. The background galaxies are played as a soft pluck sound while the bright foreground star is accompanied by a crash cymbal.<\/p>\n<p>More information about the NASA sonification project through Chandra, which is made in partnership with NASA\u2019s Universe of Learning, can be found here. The collaboration was driven by visualization scientist Kimberly Arcand (CXC), astrophysicist Matt Russo, and musician Andrew Santaguida, (both of the SYSTEM Sounds project), along with consultant Christine Malec.<\/p>\n<p>NASA\u2019s Universe of Learning materials are based upon work supported by NASA under cooperative agreement award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech\/IPAC, Center for Astrophysics | Harvard &amp; Smithsonian, and the Jet Propulsion Laboratory.<\/p>\n<p>Chandra, managed for NASA by the agency\u2019s Marshall Space Flight Center in partnership with the CXC, is one of NASA\u2019s Great Observatories, along with the\u00a0Hubble Space Telescope\u00a0and the now-retired\u00a0Spitzer Space Telescope\u00a0and\u00a0Compton Gamma Ray Observatory. It was first proposed to NASA in 1976 by Riccardo Giacconi, recipient of the 2002 Nobel Prize for Physics based on his contributions to X-ray astronomy, and Harvey Tananbaum, who would later become the first director of the Chandra X-ray Center. Chandra was named in honor of the late Nobel laureate Subrahmanyan Chandrasekhar, who earned the Nobel Prize in Physics in 1983 for his work explaining the structure and evolution of stars.<\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<p>NASA\u2019s Europa Clipper spacecraft recently got outfitted with a set of enormous solar arrays at the agency\u2019s Kennedy Space Center. Each measuring about 46\u00bd feet long and about 13\u00bd feet high, the arrays are the biggest NASA has ever developed for a planetary mission. They must be large so they can soak up as much sunlight as possible during the spacecraft\u2019s investigation of Jupiter\u2019s moon Europa, which is five times farther from the Sun than Earth is.<\/p>\n<p>The arrays have been folded up and secured against the spacecraft\u2019s main body for launch, but when they\u2019re deployed in space,\u00a0Europa Clipper\u00a0will span more than 100 feet \u2013 a few feet longer than a professional basketball court. The \u201cwings,\u201d as the engineers call them, are so big that they could only be opened one at a time in the clean room of Kennedy\u2019s Payload Hazardous Servicing Facility, where teams are readying the spacecraft for its launch period, which opens Oct. 10.\u00a0<\/p>\n<p>Meanwhile, engineers continue to assess tests conducted on the radiation hardiness of\u00a0transistors on the spacecraft. Longevity is key, because the spacecraft will journey more than five years to arrive at the Jupiter system in 2030. As it orbits the gas giant, the probe will fly by\u00a0Europa\u00a0multiple times, using a suite of\u00a0science instruments\u00a0to find out whether the ocean underneath its ice shell has conditions that could support life.<\/p>\n<p>Powering those flybys in a region of the solar system that receives only 3% to 4% of the sunlight Earth gets, each solar array is composed of five panels. Designed and built at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, and Airbus in Leiden, Netherlands, they are much more sensitive than the type of solar arrays used on homes, and the highly efficient spacecraft will make the most of the power they generate.<\/p>\n<p>At Jupiter, Europa Clipper\u2019s arrays will together provide roughly 700 watts of electricity, about what a small microwave oven or a coffee maker needs to operate. On the spacecraft, batteries will store the power to run all of the electronics, a full payload of science instruments, communications equipment, the computer, and an entire propulsion system that includes 24 engines.<\/p>\n<p>While doing all of that, the arrays must operate in extreme cold. The hardware\u2019s temperature will plunge to minus 400 degrees Fahrenheit when in Jupiter\u2019s shadow. To ensure that the panels can operate in those extremes, engineers tested them in a specialized cryogenic chamber at Li\u00e8ge Space Center in Belgium.<\/p>\n<p>\u201cThe spacecraft is cozy. It has heaters and an active thermal loop, which keep it in a much more normal temperature range,\u201d said APL\u2019s Taejoo Lee, the solar array product delivery manager. \u201cBut the solar arrays are exposed to the vacuum of space without any heaters. They\u2019re completely passive, so whatever the environment is, those are the temperatures they get.\u201d<\/p>\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube\">\n<p>\n<iframe loading=\"lazy\" title=\"Meet Europa Clipper\u2019s Solar Array \u2018Wings\u2019\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/7sa96nLa5QQ?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/p>\n<\/figure>\n<p>About 90 minutes after launch, the arrays will unfurl from their folded position over the course of about 40 minutes. About two weeks later, six antennas affixed to the arrays will also deploy to their full size. The antennas belong to the\u00a0radar instrument, which will search for water within and beneath the moon\u2019s thick ice shell, and they are enormous, unfolding to a length of 57.7 feet, perpendicular to the arrays.<\/p>\n<p>\u201cAt the beginning of the project, we really thought it would be nearly impossible to develop a solar array strong enough to hold these gigantic antennas,\u201d Lee said. \u201cIt was difficult, but the team brought a lot of creativity to the challenge, and we figured it out.\u201d<\/p>\n<p>Europa Clipper\u2019s three main science objectives are to determine the thickness of the moon\u2019s icy shell and its interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission\u2019s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet.<\/p>\n<p>Managed by Caltech in Pasadena, California, NASA\u2019s Jet Propulsion Laboratory leads the development of the Europa Clipper mission in partnership with APL for NASA\u2019s Science Mission Directorate. APL designed the main spacecraft body in collaboration with JPL and NASA\u2019s Goddard Space Flight Center. The Planetary Missions Program Office at NASA\u2019s Marshall Space Flight Center executes program management of the Europa Clipper mission.<\/p>\n<p>NASA\u2019s Launch Services Program, based at Kennedy, manages the launch service for the Europa Clipper spacecraft, which will launch on a SpaceX Falcon Heavy rocket from Launch Complex 39A at Kennedy.<\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<p>NASA\u2019s new asteroid-hunting spacecraft is taking shape at NASA\u2019s Jet Propulsion Laboratory. Called NEO Surveyor (Near-Earth Object Surveyor), this cutting-edge infrared space telescope will seek out the hardest-to-find asteroids and comets that might pose a hazard to our planet. In fact, it is the agency\u2019s first space telescope designed specifically for\u00a0planetary defense.<\/p>\n<p>Targeting launch in late 2027, the spacecraft will travel a million miles to a region of gravitational stability \u2013 called the L1 Lagrange point \u2013 between Earth and the Sun. From there, its large sunshade will block the glare and heat of sunlight, allowing the mission to discover and track near-Earth objects as they approach Earth from the direction of the Sun, which is difficult for other observatories to do. The space telescope also may reveal asteroids called\u00a0Earth Trojans, which lead and trail our planet\u2019s orbit and are difficult to see from the ground or from Earth orbit.<\/p>\n<p>NEO Surveyor relies on cutting-edge detectors that observe two bands of\u00a0infrared\u00a0light, which is invisible to the human eye. Near-Earth objects, no matter how dark,\u00a0glow brightly\u00a0in infrared as the Sun heats them. Because of this, the telescope will be able to find dark asteroids and comets, which don\u2019t reflect much visible light. It also will measure those objects, a challenging task for visible-light telescopes that have a hard time distinguishing between small, highly reflective objects and large, dark ones.<\/p>\n<p>\u201cNEO Surveyor is optimized to help us to do one specific thing: enable humanity to find the most hazardous asteroids and comets far enough in advance so we can do something about them,\u201d said Amy Mainzer, survey director for NEO Surveyor and a professor at the University of California, Los Angeles. \u201cWe aim to build a spacecraft that can find, track, and characterize the objects with the greatest chance of hitting Earth. In the process, we will learn a lot about their origins and evolution.\u201d<\/p>\n<p>The spacecraft\u2019s only instrument is its telescope. About the size of a washer-and-dryer set, the telescope\u2019s blocky aluminum body, called the optical bench, was built in a JPL clean room. Known as a three-mirror anastigmat telescope, it will rely on curved mirrors to focus light onto its infrared detectors in such a way that minimizes optical aberrations.<\/p>\n<p>\u201cWe have been carefully managing the fabrication of the spacecraft\u2019s telescope mirrors, all of which were received in the JPL clean room by July,\u201d said Brian Monacelli, principal optical engineer at JPL. \u201cIts mirrors were shaped and polished from solid aluminum using a diamond-turning machine. Each exceeds the mission\u2019s performance requirements.\u201d<\/p>\n<p>Monacelli inspected the mirror surfaces for debris and damage, then JPL\u2019s team of optomechanical technicians and engineers attached the mirrors to the telescope\u2019s optical bench in August. Next, they will measure the telescope\u2019s performance and align its mirrors.<\/p>\n<p>Complementing the mirror assembly are the telescope\u2019s mercury-cadmium-telluride detectors, which are similar to the detectors used by NASA\u2019s recently retired\u00a0NEOWISE\u00a0(short for Near-Earth Object Wide-field Infrared Survey Explorer) mission. An advantage of these detectors is that they don\u2019t necessarily require cryogenic coolers or cryogens to lower their operational temperatures in order to detect infrared wavelengths. Cryocoolers and cryogens can limit the lifespan of a spacecraft. NEO Surveyor will instead keep its cool by using its large sunshade to block sunlight from heating the telescope and by occupying an orbit beyond that of the Moon, minimizing heating from Earth.<\/p>\n<p>The telescope will eventually be installed inside the spacecraft\u2019s instrument enclosure, which is being assembled in JPL\u2019s historic\u00a0High Bay 1 clean room\u00a0where NASA missions such as Voyager, Cassini, and Perseverance were constructed. Fabricated from dark composite material that allows heat to escape, the enclosure will help keep the telescope cool and prevent its own heat from obscuring observations.<\/p>\n<p>Once it is completed in coming weeks, the enclosure will be tested to make sure it can withstand the rigors of space exploration. Then it will be mounted on the back of the sunshade and atop the electronic systems that will power and control the spacecraft.<\/p>\n<p>\u201cThe entire team has been working hard for a long time to get to this point, and we are excited to see the hardware coming together with contributions from our institutional and industrial collaborators from across the country,\u201d said Tom Hoffman, NEO Surveyor\u2019s project manager at JPL. \u201cFrom the panels and cables for the instrument enclosure to the detectors and mirrors for the telescope \u2014 as well as components to build the spacecraft \u2014 hardware is being fabricated, delivered, and assembled to build this incredible observatory.\u201d<\/p>\n<p>Assembly of NEO Surveyor can be viewed 24 hours a day, seven days a week, via\u00a0JPL\u2019s live cam.<\/p>\n<p>The NEO Surveyor mission marks a major step for NASA toward reaching its U.S. Congress-mandated goal to discover and characterize at least 90% of the near-Earth objects more than 460 feet across that come within 30 million miles of our planet\u2019s orbit. Objects of this size can cause significant regional damage, or worse, should they impact the Earth.<\/p>\n<p>The mission is tasked by NASA\u2019s Planetary Science Division within the Science Mission Directorate; program oversight is provided by the Planetary Defense Coordination Office, which was established in 2016 to manage the agency\u2019s ongoing efforts in planetary defense. NASA\u2019s Planetary Missions Program Office at the agency\u2019s Marshall Space Flight Center provides program management for NEO Surveyor.<\/p>\n<p>The project is being developed by JPL and is led by survey director Amy Mainzer at UCLA. Established aerospace and engineering companies have been contracted to build the spacecraft and its instrumentation, including BAE Systems, Space Dynamics Laboratory, and Teledyne. The Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder will support operations, and IPAC-Caltech in Pasadena, California, is responsible for processing survey data and producing the mission\u2019s data products. Caltech manages JPL for NASA.<\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<p>NASA will provide live coverage of the upcoming activities for Boeing\u2019s Starliner spacecraft departure from the International Space Station and return to Earth. The uncrewed spacecraft will depart from the orbiting laboratory for a landing at White Sands Space Harbor in New Mexico.<\/p>\n<p>Starliner is scheduled to autonomously undock from the space station at approximately 5:04 p.m. CDT Sept. 6, to begin the journey home, weather conditions permitting. NASA and Boeing are targeting approximately 11:03 p.m. Sept. 6 for the landing and conclusion of the flight test.<\/p>\n<p>NASA\u2019s live coverage of return and related activities will stream on\u00a0NASA+, the\u00a0NASA app, and the agency\u2019s\u00a0website. Learn how to\u00a0stream\u00a0NASA programming through a variety of platforms including social media.<\/p>\n<p>NASA astronauts Butch Wilmore and Suni Williams launched aboard Boeing\u2019s Starliner spacecraft on June 5 for its first crewed flight, arriving at the space station on June 6. As Starliner approached the orbiting laboratory, NASA and Boeing identified helium leaks and experienced issues with the spacecraft reaction control thrusters. For the safety of the astronauts, NASA announced on Aug. 24 that Starliner will return to Earth from the station without a crew. Wilmore and Williams will remain aboard the station and return home in February 2025 aboard the SpaceX Dragon spacecraft with two other crew members assigned to NASA\u2019s SpaceX Crew-9 mission.<\/p>\n<p><strong><strong>\u203a Back to Top<\/strong><\/strong><\/p>\n<\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/www.nasa.gov\/centers-and-facilities\/marshall\/the-marshall-star-for-september-4-2024\/?rand=772114\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>NASA is making strides with the\u00a0Artemis campaign\u00a0as key components for the SLS (Space Launch System) rocket continue to make their way to\u00a0NASA\u2019s Kennedy Space Center. Teams with NASA and Boeing&hellip; <\/p>\n","protected":false},"author":1,"featured_media":788364,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[4],"tags":[],"class_list":["post-788363","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-NASA"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/788363","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=788363"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/788363\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/788364"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=788363"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=788363"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=788363"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}