Members Can Post Anonymously On This Site
Receipt of a Small Apollo 16 Regolith Dust Sample for the Dusty Plasma Lab
-
Similar Topics
-
By European Space Agency
ESA's Prospect package, including drill and a miniaturised laboratory, will fly to the Moon’s South Polar region in search of volatiles, including water ice, as part of NASA’s Commercial Lunar Payload Services initiative.
View the full article
-
By NASA
NASA Earth Observatory image by Lauren Dauphin, using VIIRS data from NASA EOSDIS LANCE, GIBS/Worldview, and the Suomi National Polar-orbiting Partnership The Suomi NPP satellite acquired this image of a plume of Saharan dust as winds lofted it over the Atlantic Ocean on Aug. 24, 2024.
The Sahara Desert is Earth’s largest source of airborne dust, and the particles can travel for thousands of miles. From late spring to early fall, it is common for the dry, dusty Saharan Air Layer to carry the particles westward across the Atlantic Ocean high in the atmosphere. Saharan Air Layer activity subsides after mid-August, according to NOAA, making it less likely that the plume shown here is bound for a transoceanic journey. Instead, it arcs to the north after blowing out over the ocean. Earlier in the summer, however, several clouds of fine dust from the Sahara reached the United States, creating hazy skies over Texas.
Read more about Saharan dust and why it’s interesting to scientists.
Text Credit: Lindsey Doermann
Image Credit: NASA/Lauren Dauphin, using VIIRS data from NASA EOSDIS LANCE, GIBS/Worldview, and the Suomi National Polar-orbiting Partnership
View the full article
-
By NASA
Earlier this month, nine small businesses received 2023 NASA Small Business Innovation Research (SBIR) Ignite Phase II awards to further develop technologies that may be used in the agency’s missions and in the commercial space industry.
The SBIR Ignite Phase II awardees, who will receive up to $850,000 to fund their projects, are developing technology capabilities in the detection of wildfires, support for water management in agriculture, in-space debris detection, mineral mining from lunar regolith, in-space production, and more. These capabilities are vital to supporting deep space exploration, low Earth orbit missions, and preserving life on our home planet for the benefit of all. The businesses initially were selected for Phase I awards in 2023 and provided six months and up to $150,000 to prove their concepts before competing for Phase II.
“We want to support innovators across the aerospace industry because their technologies have the potential to make a big impact in the commercial market. A rich and diverse marketplace creates more opportunity for us all. These Phase II awards illuminate a clear path for a unique range of technologies that we believe will positively influence the lives of all Americans.”
Jason L. Kessler
NASA SBIR/STTR Program Executive
The SBIR Ignite pilot initiative supports product-driven small businesses, startups, and entrepreneurs that have commercialization at the forefront of their innovation strategies and processes but that are not targeting NASA as a primary customer. The pilot initiative provides funding and other support to mitigate risk in technologies that have strong commercial potential by offering lower barriers to entry, a streamlined review and selection process, and accelerated technology development and awards as compared to the NASA SBIR program’s main solicitation. It also focuses on helping make participating companies more appealing to investors, customers, and partners, while fulfilling SBIR’s mission of increasing commercialization of innovations derived from federal research and development.
While the agency’s main Small Business Innovation Research and Small Business Technology Transfer solicitations focus on technologies with potential for infusion in both NASA missions and commercialization in the marketplace, the SBIR Ignite opportunity is less prescriptive and focuses on topics that are relevant to emerging commercial markets in aerospace, such as accelerating in-space production applications in low Earth orbit.
The awarded companies are:
Astral Forge, LLC, Palo Alto, California Astrobotic Technology Inc., Pittsburgh Benchmark Space Systems, Burlington, Vermont Brayton Energy, LLC, Hampton, New Hampshire Channel-Logistics LLC dba Space-Eyes, Miami GeoVisual Analytics, Westminster, Colorado Space Lab Technologies, LLC, Boulder, Colorado Space Tango, Lexington, Kentucky VerdeGo Aero, De Leon Springs, Florida
The third year of NASA Small Business Innovation Research (SBIR) Ignite is underway, as the 2024 SBIR Ignite Phase I solicitation closed on July 30, 2024. Those selections are expected to be announced Fall 2024.
NASA’s Small Business Innovation Research and Small Business Technology Transfer program is part of NASA’s Space Technology Mission Directorate and is managed by NASA’s Ames Research Center in Silicon Valley.
View the full article
-
By NASA
As part of an asteroid sample exchange, NASA has transferred to JAXA (Japan Aerospace Exploration Agency) a portion of the asteroid Bennu sample collected by the agency’s OSIRIS-REx mission. The sample was officially handed over by NASA officials during a ceremony on Aug. 22 at JAXA’s Sagamihara, Japan, campus.
The signature exchange for the Bennu sample transfer took place on Aug. 22, 2024, at JAXA’s (Japan Aerospace Exploration Agency) Institute of Space and Astronautical Science, Sagamihara Campus.JAXA This asteroid sample transfer follows the November 2021 exchange where JAXA transferred to NASA a portion of the sample retrieved from asteroid Ryugu by its Hayabusa2 spacecraft. This agreement allows NASA and JAXA to share achievements and promote scientific and technological cooperation on asteroid sample return missions. The scientific goals of the two missions are to understand the origins and histories of primitive, organic-rich asteroids and what role they may have played in the formation of the planets.
“We value our continued collaboration with JAXA on asteroid sample return missions to both increase our science return and reduce risk on these and other missions,” said Kathleen Vander Kaaden, chief scientist for astromaterials curation in the Science Mission Directorate at NASA Headquarters in Washington. “JAXA has extensive curation capabilities, and we look forward to what we will learn from the shared analysis of the OSIRIS-REx samples.”
The Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer, or OSIRIS-REx, spacecraft delivered 4.29 ounces (121.6 grams) of material from Bennu, more than double the mission’s mass requirement, as well as 24 steel Velcro® pads containing dust from the contact with Bennu. As part of the agreement, the Astromaterials Research and Exploration Science Division at NASA’s Johnson Space Center in Houston transferred to JAXA 0.023 ounces (0.66 grams) of the Bennu sample, equaling 0.55% of the total sample mass, and one of the 24 contact pads.
Hayabusa2 collected 0.19 ounces (5.4 grams) of Ryugu between two samples and, in 2021, JAXA provided NASA with 23 millimeter-sized grains plus aggregate sample material from Ryugu, enabling both countries to get the most out of the samples and share the responsibility of sample curation.
JAXA’s portion of the Bennu samples will be housed in the newly expanded clean rooms in the extraterrestrial sample curation center on the JAXA Sagamihara campus. The JAXA team received the samples enclosed in non-reactive nitrogen gas and will open them in similarly nitrogen-filled clean chambers, accessed with air-tight gloves. JAXA will now work to create an initial description of the sample, including weight measurements, imaging with both visible light and infrared light microscopes, and infrared spectroscopy. The sample will then be distributed through a competitively selected process for detailed analysis at other research institutes to study the differences and similarities between asteroids Bennu and Ryugu.
JAXA “Thank you for safely bringing the precious asteroid samples from Bennu to Earth and then to Japan,” said Tomohiro Usui, Astromaterials Science Research Group Manager, Institute of Space and Astronautical Science, JAXA. “As fellow curators, we understand the tension and responsibility that accompany these tasks. Now, it is our turn at JAXA. We will go ahead with our plans to derive significant scientific outcomes from these valuable samples.”
Asteroids are debris left over from the dawn of the solar system. The Sun and its planets formed from a cloud of dust and gas about 4.6 billion years ago, and asteroids are thought to date back to the first few million years of our solar system’s history. Sample return missions like OSIRIS-REx and Hayabusa2 help provide new data on how the solar system’s evolution unfolded.
Initial analysis of the Bennu samples has revealed dust rich in carbon and nitrogen. Members of the OSIRIS-REx sample analysis team have also found evidence of organic molecules and minerals bearing phosphorous and water, which together could indicate the building blocks essential for life.
Both the Bennu sample and the asteroid Ryugu sample delivered by JAXA’s Hayabusa2 mission appear to have come from an ancient parent object formed beyond the current orbit of Saturn that was broken up and transported into the inner solar system. The differences between these asteroids are emerging as the detailed chemistry is analyzed.
NASA’s Goddard Space Flight Center in Greenbelt, Maryland, provided overall mission management, systems engineering, and the safety and mission assurance for OSIRIS-REx. Dante Lauretta of the University of Arizona, Tucson, is the principal investigator. The university leads the science team and the mission’s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft and provided flight operations. Goddard and KinetX Aerospace were responsible for navigating the OSIRIS-REx spacecraft. Curation for OSIRIS-REx takes place at NASA Johnson. International partnerships on this mission include the OSIRIS-REx Laser Altimeter instrument from CSA (Canadian Space Agency) and asteroid sample science collaboration with JAXA’s Hayabusa2 mission. OSIRIS-REx is the third mission in NASA’s New Frontiers Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington.
Find more information about NASA’s OSIRIS-REx mission at:
https://science.nasa.gov/mission/osiris-rex
-end-
News Media Contacts
Wynn Scott
NASA’s Johnson Space Center, Houston
281-910-6835
wynn.b.scott@nasa.gov
Karen Fox / Alana Johnson
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov
View the full article
-
By NASA
On Aug. 10, 1969, Apollo 11 astronauts Neil A. Armstrong, Michael Collins, and Edwin E. “Buzz” Aldrin completed their 21-day quarantine after returning from the Moon. The historic nature of their mission resulted in a very busy postflight schedule for Armstrong, Collins, and Aldrin, starting with celebrations in New York, Chicago, Los Angeles, and Houston. Scientists continued to examine the lunar samples the Apollo 11 astronauts returned from the Sea of Tranquility. NASA set its sights on additional lunar landing missions, announcing plans for a pinpoint landing by Apollo 12 in November 1969 that also included visiting the robotic Surveyor 3 that landed on the Moon in 1967. The agency announced the crews for the Apollo 13 and 14 missions planned for 1970. Including prime and backup crews, NASA had 18 astronauts training for lunar landing missions. Support astronauts brought that number to 32.
Apollo 11
Following their return from the Moon, Armstrong, Collins, and Aldrin completed their 21-day quarantine in the Lunar Receiving Laboratory (LRL) at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston. During their stay in the LRL, they worked on their pilot reports, conducted postflight debriefs including with the Apollo 12 crew, and Armstrong celebrated his 39th birthday. On the evening of Aug. 10, they left the relative quiet of the LRL for a very hectic next few months. After spending a day reuniting with their families, the three reported back to their offices and held their postflight press conference on Aug. 12. The next day, they flew first to New York for a massive ticker tape parade, then on to Chicago for another big parade, ending the day in Los Angeles with a state dinner hosted by President Richard M. Nixon and attended by most active astronauts, members of Congress, 44 state governors, and 83 foreign ambassadors. They returned to Houston for a welcome home parade on Aug. 16, ending the day with a barbecue party and a tribute to the entire NASA team in the Astrodome, emceed by Frank Sinatra. Meanwhile, on Aug. 14, engineers shipped the Command Module Columbia to its manufacturer, the North American Rockwell plant in Downey, California, for postflight inspections. Scientists in the LRL eagerly continued their examinations of the 48 pounds of lunar material the Apollo 11 astronauts returned from the Sea of Tranquility.
Left: In the Lunar Receiving Laboratory (LRL) at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston, Apollo 11 astronauts Neil A. Armstrong, left, Michael Collins, and Edwin E. “Buzz” Aldrin line up for food in the LRL’s dining area. Middle: Buzz, left, Mike, and Neil enjoy a meal together in the LRL’s dining room. Right: Neil celebrates his 39th birthday in the LRL.
Left: NASA engineer John K. Hirasaki opens the hatch to the Apollo 11 Command Module Columbia for the first time in the Lunar Receiving Laboratory (LRL) at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston. Middle: Mike Collins sits in Columbia’s hatch in the LRL. Right: While still aboard the U.S.S. Hornet, Mike wrote this inscription inside Columbia.
Collins’ inscription inside Columbia, first written while aboard the U.S.S. Hornet, and retraced in the LRL:
Spacecraft 107, alias Apollo 11, alias “Columbia”
The Best Ship to Come Down the Line
God Bless Her.
Michael Collins CMP
Aug. 5, 1969. In the Lunar Receiving Laboratory, scientists open the second Apollo 11 Lunar Sample Return Container and begin to examine the rock and soil samples.
Left: On Aug. 10, 1969, Buzz, left, Mike, and Neil exit the Lunar Receiving Laboratory at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston, ending their 21-day quarantine. Middle: Morning of Aug. 12, Neil reports to work at his office in MSC’s Building 4. Right: Afternoon of Aug. 12, Buzz, left, Neil, and Mike meet the press in MSC’s auditorium.
Armstrong’s comments to open the press conference:
“It was our pleasure to participate in one great adventure. It’s an adventure that took place, not just in the month of July, but rather one that took place in the last decade. We … had the opportunity to share that adventure over its developing and unfolding in the past months and years. It’s our privilege today to share with you some of the details of that final month of July that was certainly the highlight, for the three of us, of that decade.”
Aug. 13, 1969. Left: An estimated four million people attend the ticker tape parade in New York City for the Apollo 11 astronauts. Middle: The ticker tape parade in Chicago drew two million people. Right: The Apollo 11 astronauts and their wives at the official state dinner in Los Angeles, hosted by President Richard M. Nixon.
Left: Aug. 14, 1969. NASA Administrator Thomas O. Paine, left, accompanies Buzz, Mike, and Neil on the plane back to Houston. Middle: Aug. 16. Ticker tape parade in downtown Houston attended by 250,000 people. Right: Aug. 16. Buzz, left, Neil, and Mike with emcee Frank Sinatra during the barbecue party in the Houston Astrodome.
Left: On Aug. 14, at Houston’s Ellington Air Force Base, workers load the Apollo 11 Command Module Columbia into a Super Guppy for transport to the North American Rockwell plant in Downey, California. Middle: Workers in Downey inspect Columbia on Aug. 19. Right: Workers prepare to place Columbia in a chamber to bakeout any residual moisture to ready it for public display.
Apollo 11 science experiments. Left: Neil rolled up the Solar Wind Composition experiment at the end of the spacewalk and placed it inside the Apollo Lunar Sample Return Container that arrived in the Lunar Receiving Laboratory on July 26, 1969. Middle: Astronomers sent the first successful beam to the Laser Ranging Retroreflector on Aug. 1, 1969, and it remains available for use to this day. Right: The Passive Seismic Experiment returned useful data for three weeks but stopped responding to commands on Aug. 24, 1969, most likely due to overheating in the lunar Sun.
Apollo 12
At the time Apollo 11 returned from its historic journey, NASA had plans for nine more Apollo Moon landing missions. On July 29, Apollo Program Director Samuel C. Phillips at NASA Headquarters in Washington, D.C., announced the launch date, Nov. 14, 1969, and the landing site, in the Ocean of Storms, for Apollo 12. The main goals of this second lunar landing included a precision touchdown near the Surveyor 3 spacecraft that landed there in April 1967, and an expanded science program conducted during two spacewalks, including the deployment of the first Apollo Lunar Surface Experiment Package (ALSEP), a suite of science instruments. The Apollo 12 prime crew of Commander Charles “Pete” Conrad, Command Module Pilot (CMP) Richard F. Gordon, and Lunar Module Pilot (LMP) Alan L. Bean and their backups David R. Scott, Alfred M. Worden, and James B. Irwin, began training after their assignment in April. In addition to rehearsing aspects of their flight in mission simulators, they practiced for the descent and precision landing, for the two spacewalks planned during their 31.5-hour lunar surface stay, including visiting and examining Surveyor 3, and for the expanded geology exploration. The latter included a three-day geology field trip to Hawaii with simulated lunar traverses. At NASA’s Jet Propulsion Laboratory in Pasadena, California, the astronauts received a detailed briefing on the Surveyor spacecraft. At NASA’s Kennedy Space Center (KSC) in Florida, workers had already assembled their Saturn V rocket, with rollout to Launch Pad 39A planned for early September. The U.S. Navy chose the U.S.S. Hornet (CVS-12), the carrier that successfully recovered Apollo 11, to reprise its role as prime recovery ship for Apollo 12.
Left: Lunar front side showing the landing sites for Apollo 11 and 12. Right: Surveyor 3 took this panorama of its landing site in April 1967, also the targeted site for Apollo 12.
Left: Apollo 12 astronauts Charles “Pete” Conrad, left, and Alan L. Bean at the Lunar Landing Research Facility (LLRF) at NASA’s Langley Research Center in Hampton, Virginia. Middle left: Apollo 12 backup astronaut David R. Scott at the LLRF. Middle right: Conrad, left, and Bean during the Aug. 9-11 geology field trip to Hawaii. Right: Conrad practices opening an Apollo Lunar Sample Return Container during simulated one-sixth gravity aboard a KC-135 aircraft.
Apollo 13 and 14
On Aug. 6, 1969, NASA announced the crews for Apollo 13 and 14, the third and fourth Moon landing missions. At the time of the announcement, Apollo 13 had a planned launch date in March 1970 and a proposed landing site at the Fra Mauro region in the lunar highlands, the first landing site not in the relatively flat lunar maria. Apollo 14 aimed for a July 1970 mission with the Crater Censorinus area in the lunar highlands to the southeast of the Sea of Tranquility as a tentative landing site. Plans for both missions called for two lunar surface excursions totaling about six hours with a lunar stay duration of 35 hours. As on Apollo 12, the crews planned to deploy an ALSEP suite of science instruments, in addition to conducting the geology field work of documenting and collecting rock and soil samples for return to scientists on Earth for analysis.
The Apollo 13 crew of James A. Lovell, left, Thomas K. “Ken” Mattingly, and Fred W. Haise.
The prime crew for Apollo 13 consisted of Commander James A. Lovell, CMP Thomas K. “Ken” Mattingly, and LMP Fred W. Haise. Lovell would make his fourth space mission aboard Apollo 13, having flown on Gemini VII and XII as well as orbiting the Moon during Apollo 8 – making him the first person to travel to the Moon twice. Neither Mattingly nor Haise had flown in space before, although Haise had served with Lovell on the Apollo 11 backup crew. The Apollo 13 backup crew consisted of John W. Young, John L. Swigert, and Charles M. Duke. Young had flown three previous missions, Gemini 3 and X and more recently aboard Apollo 10, the Moon landing dress rehearsal flight. Swigert and Duke had no spaceflight experience, although Duke served as capsule communicator during Apollo 10 as well as during the Apollo 11 Moon landing.
Left: The Saturn V for Apollo 13 rolls out of the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida to relocate it from High Bay 2 to High Bay 1. Right: The Apollo 13 Saturn V rolls back in to High Bay 1 of the VAB.
Flight hardware for Apollo 13 had already arrived at KSC. Workers in the Vehicle Assembly Building (VAB) completed stacking of the three Saturn V rocket stages in High Bay 2 on July 31. They added a boilerplate Apollo spacecraft to the top of the rocket, and in a roll-around maneuver on Aug. 8, the stack left the VAB, crawled to the other side of the building, and rolled back inside to High Bay 1. North American Rockwell delivered the Command and Service Modules to KSC on June 26, where workers in the Manned Spacecraft Operations Building (MSOB) mated the two modules four days later in preparation for preflight testing in altitude chambers. The Lunar Module (LM) ascent and descent stages arrived at KSC on June 27 and 28, respectively, from their manufacturer, the Grumman Aircraft Corporation in Bethpage, New York. Following a docking test between the CM and LM, workers in the MSOB mated the two stages of the LM on July 15.
The Apollo 14 crew of Alan B. Shepard, left, Stuart A. Roosa, and Edgar D. Mitchell.
NASA designated Commander Alan B. Shepard, CMP Stuart A. Roosa, and LMP Edgar D. Mitchell as the prime crew for Apollo 14. Shepard, the first American in space when he launched aboard his Freedom 7 spacecraft in May 1961, recently returned to flight status after a surgical intervention cured his Ménière’s disease, an inner ear disorder. Neither Roosa nor Mitchell had spaceflight experience. The backup crew consisted of Eugene A. Cernan, Ronald E. Evans, and Joe H. Engle. Cernan had flown in space twice before, on Gemini IX and more recently on Apollo 10. Evans and Engle had not flown in space before, although Engle earned astronaut wings as a pilot with the U.S. Air Force flying the X-15 rocket plane above the 50-mile altitude required to qualify as an astronaut on three of his 16 flights.
Left: Apollo 14 astronauts Alan B. Shepard, center, and Edgar D. Mitchell, in baseball cap, during the Idaho geology field trip. Right: Apollo 14 backup crew members Eugene A. Cernan, left, and Joe H. Engle during the Idaho geology field trip.
The Apollo 14 astronauts jumped right into their geology training. On Aug. 14, Shepard, Mitchell, and Engle spent the day at the United States Geological Service’s (USGS) Crater Field near Flagstaff, Arizona, including getting a geologist’s lecture on the mechanisms of crater formation. On Aug. 22 and 23, Cernan joined them on a geology field trip to Idaho, where they visited Craters of the Moon National Monument, Butte Crater lava tubes, Ammon pumice quarries, and the Wapi volcanic fields. Geologists chose these sites for training because at the time Apollo 14 planned to visit a presumed volcanic area on the Moon.
NASA management changes
Left: Samuel C. Phillips, Apollo Program Director at NASA Headquarters in Washington, D.C., during the Apollo 11 launch in the Launch Control Center at NASA’s Kennedy Space Center (KSC) in Florida. Middle left: Rocco A. Petrone, director of launch operations at KSC, seen here at the Apollo 11 rollout, succeeded Phillips. Middle right: George S. Trimble, left, deputy director of the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston, with MSC Director Robert R. Gilruth in 1967. Right: Christopher C. Kraft, director of flight operations at MSC, seen here in Mission Control following the Apollo 11 splashdown, succeeded Trimble.
Several changes in senior NASA leadership took place following Apollo 11. At NASA Headquarters in Washington, D.C., Phillips retired as Apollo Program Director, having served in that position since 1964, and returned to the U.S. Air Force. Rocco A. Petrone, director of launch operations at KSC since 1966, succeeded him. George S. Trimble announced his retirement as MSC deputy director effective Sept. 30, having served in that role since October 1967. In November 1969, MSC Director Robert R. Gilruth named Christopher C. Kraft to succeed Trimble as his deputy.
To be continued …
News from around the world in August 1969:
August 2 – President Nixon the first sitting U.S. president to visit a communist capital when he meets with Romanian President Nicolai Ceausescu in Bucharest.
August 5 – Mariner 7 returns close-up images during its fly-by of Mars.
August 14 – NASA accepts seven pilots from the U.S. Air Force’s canceled Manned Orbiting Laboratory as its Group 7 astronauts.
August 15-18 – Three-day Woodstock music festival in Bethel, New York, draws nearly half a million attendees.
August 21 – The first GAP store opens in San Francisco.
Explore More
7 min read 55 Years Ago: NASA Group 7 Astronaut Selection
Article 6 days ago 5 min read Celebrating NASA’s Coast Guard Astronauts on Coast Guard Day
Article 3 weeks ago 20 min read MESSENGER – From Setbacks to Success
Article 3 weeks ago View the full article
-
-
Check out these Videos
Recommended Posts
Join the conversation
You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.