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NASA has awarded the NASA Academic Mission Services 2 (NAMS-2) contract to Crown Consulting Inc., of Arlington, Virginia, to provide the agency’s Ames Research Center in California’s Silicon Valley, aeronautics and exploration technology research and development support.

NAMS-2 is a single award hybrid cost-plus-fixed-fee indefinite-delivery indefinite-quantity contract with a maximum potential value of $121 million. The contract begins Tuesday, Oct. 1, 2024, with a 60-day phase-in period, followed by a two-year base period, and options to extend performance through November 2029.

Under this contract, the company will support a broad scope of scientific research and development of new and emerging capabilities and technologies associated with air traffic management, advanced technology, nanoelectronics, and prototype software in support of the Aeronautics Directorate and the Exploration Technology Directorate at NASA Ames. The work also will focus on the improvement of aircraft and airspace safety, as well as the transition of advanced aeronautics technologies into future air vehicles.

For information about NASA and agency programs, visit:

https://www.nasa.gov

-end-

Roxana Bardan
Headquarters, Washington
202-358-1600
roxana.bardan@nasa.gov

Rachel Hoover
Ames Research Center, Silicon Valley, Calif.
rachel.hoover@nasa.gov
650-604-4789

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Details Last Updated Sep 13, 2024 LocationAmes Research Center

The waxing gibbous Moon is pictured from the International Space Station as it orbited 265 miles above the U.S. state of Minnesota on Dec. 17, 2021.

NASA, ESA/Matthias Maurer

An astronaut aboard the International Space Station snapped this picture of the Moon as the station orbited 265 miles above the U.S. state of Minnesota on Dec. 17, 2021.

Astronauts aboard the orbital lab take images using handheld digital cameras, usually through windows in the station’s cupola, for Crew Earth Observations. Crew members have produced hundreds of thousands of images of the Moon and Earth’s land, oceans, and atmosphere.

On Saturday, Sept. 14, 2024, International Observe the Moon Night, everyone on Earth is invited to learn about lunar science, participate in celestial observations, and honor cultural and personal connection to the Moon. Find an event to join in the celebration.

Image credit: NASA, ESA/Matthias Maurer

The Sun rises above the Flight Research Building at NASA’s Glenn Research Center in Cleveland.Credit: NASA

Editor’s note: This media advisory was updated Friday, Sept. 13, 2024, with a correct phone number for the media contact at NASA’s Glenn Research Center.

NASA‘s Watts on the Moon Challenge, designed to advance the nation’s lunar exploration goals under the Artemis campaign by challenging United States innovators to develop breakthrough power transmission and energy storage technologies that could enable long-duration Moon missions, concludes on Friday, Sept. 20, at the Great Lakes Science Center in Cleveland.

“For astronauts to maintain a sustained presence on the Moon during Artemis missions, they will need continuous, reliable power,” said Kim Krome-Sieja, acting program manager, Centennial Challenges at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “NASA has done extensive work on power generation technologies. Now, we’re looking to advance these technologies for long-distance power transmission and energy storage solutions that can withstand the extreme cold of the lunar environment.”

The technologies developed through the Watts on the Moon Challenge were the first power transmission and energy storage prototypes to be tested by NASA in an environment that simulates the extreme cold and weak atmospheric pressure of the lunar surface, representing a first step to readying the technologies for future deployment on the Moon. Successful technologies from this challenge aim to inspire, for example, new approaches for helping batteries withstand cold temperatures and improving grid resiliency in remote locations on Earth that face harsh weather conditions.

Media and the public are invited to attend the grand finale technology showcase and awards ceremony for the $5 million, two-phase competition. U.S. and international media interested in covering the event should confirm their attendance with Lane Figueroa by 3 p.m. CDT Tuesday, Sept. 17, at: lane.e.figueroa@nasa.gov. NASA’s media accreditation policy is available online. Members of the public may register as an attendee by completing this form, also by Friday, Sept. 17.

During the final round of competition, finalist teams refined their hardware and delivered a full system prototype for testing in simulated lunar conditions at NASA’s Glenn Research Center in Cleveland. The test simulated a challenging power system scenario where there are six hours of solar daylight, 18 hours of darkness, and the user is three kilometers from the power source.

“Watts on the Moon was a fantastic competition to judge because of its unique mission scenario,” said Amy Kaminski, program executive, Prizes, Challenges, and Crowdsourcing, Space Technology Mission Directorate at NASA Headquarters in Washington. “Each team’s hardware was put to the test against difficult criteria and had to perform well within a lunar environment in our state-of-the-art thermal vacuum chambers at NASA Glenn.”

Each finalist team was scored based on Total Effective System Mass (TESM), which determines how the system works in relation to its mass. At the awards ceremony, NASA will award $1 million to the top team who achieves the lowest TESM score, meaning that during testing, that team’s system produced the most efficient output-to-mass ratio. The team with the second lowest mass will receive $500,000. The awards ceremony stream live on NASA Glenn’s YouTube channel and NASA Prize’s Facebook page.

The Watts on the Moon Challenge is a NASA Centennial Challenge led by NASA Glenn. NASA Marshall manages Centennial Challenges, which are part of the agency’s Prizes, Challenges, and Crowdsourcing program in the Space Technology Mission Directorate. NASA has contracted HeroX to support the administration of this challenge.

For more information on NASA’s Watts on the Moon Challenge, visit:

https://www.nasa.gov/wattson

-end- 

Jasmine Hopkins
Headquarters, Washington
321-432-4624
jasmine.s.hopkins@nasa.gov

Lane Figueroa
Marshall Space Flight Center, Huntsville, Ala.
256-932-1940
lane.e.figueroa@nasa.gov

Brian Newbacher
Glenn Research Center, Cleveland
216-469-9726
brian.t.newbacher@nasa.gov

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Details Last Updated Sep 13, 2024 EditorJessica TaveauLocationNASA Headquarters Related Terms

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Sols 4302-4303: West Side of Upper Gediz Vallis, From Tungsten Hills to the Next Rocky Waypoint This photo taken by NASA’s Mars rover Curiosity of ‘Balloon Dome’ covers a low dome-like structure formed by the light-toned slab-like rocks. This image was taken by Left Navigation Camera aboard Curiosity on Sol 4301 — Martian day 4,301 of the Mars Science Laboratory mission — on Sept. 11, 2024, at 09:14:42 UTC. NASA/JPL-Caltech

Earth planning date: Wednesday, Sept. 11, 2024

The rover is on its way from the Tungsten Hills site to the next priority site for Gediz Vallis channel exploration, in which we plan to get in close enough for arm science to one of the numerous large dark-toned “float” blocks in the channel and also to one of the light-toned slabs.  We have seen some dark blocks in the channel that seem to be related to the Stimson formation material that the rover encountered earlier in the mission, but some seem like they could be something different. We don’t think any of them originated in the channel so they have to come from somewhere higher up that the rover hasn’t been, and we’re interested in how they were transported down into the channel.

We aren’t there yet, but the 4302-4303 plan’s activities include some important longer-range characterization of the dark-toned and light-toned materials via imaging. Context for the future close-up science on the dark-toned blocks will be provided by the Mastcam mosaics named “Bakeoven Meadow” and “Balloon Dome.”  The broad Balloon Dome mosaic also covers a low dome-like structure formed by the light-toned slab-like rocks (pictured).  Smaller mosaics will cover a pair of targets that include contacts where other types of light-toned and dark-toned material occur next to each other in the same block: “Rattlesnake Creek” which appears to be in place, and “Casa Diablo Hot Springs,” which is a float.

The rover’s arm workspace provided an opportunity for present-day aeolian science on the sandy-looking ripple, Sandy Meadow. Mastcam stereo imaging will document the shape of the ripple, while a suite of high-resolution MAHLI images will tell us something about the particle size of the grains in it.  The modern environment will also be monitored via a suprahorizon observation, a dust devil survey, and imaging of the rover deck to look for dust movement.

The workspace included small examples of the dark float blocks, so the composition of one of them will be measured by both APXS and ChemCam LIBS as targets “Lucy’s Foot Pass” and “Colt Lake” respectively.

In the meantime, the Mastcam Boneyard Meadow mosaic will provide a look back at the Tungsten Hills dark rippled block along its bedding plane to try to narrow down the origin of the ripples and the potential roles of water vs. wind in their formation.

Communication remains a challenge for the rover in this location. During planning, the rover’s drive was shifted from the second sol to the first sol in order to increase the downlink data volume available for the post-drive imaging, thereby enabling better planning at the science waypoint we expect to reach in the weekend plan. However, maintaining communications will require the rover to end its drive in a narrow range of orientations, which could make approaching our next science target a bit tricky.  We’ll find out on Friday!

Written by: Lucy Lim, Planetary Scientist at NASA Goddard Space Flight Center
Edited by: Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory

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Image Credit: BitGrit

The Digital Information Platform (DIP) Sub-Project of Air Traffic Management – eXploration (ATM-X) is seeking to make available in the National Airspace System a variety of live data feeds and services built on that data. The goal is to allow external partners to build advanced, data-driven services using this data and to make these services available to flight operators, who will use these capabilities to save fuel and avoid delays. Different wind directions, weather conditions at or near the airport, inoperative runway, etc., affects the runway configurations to be used and impacts the overall arrival throughputs. Knowing the arrival runway and its congestion level ahead of time will enable aviation operators to perform better flight planning and improve the flight efficiency. This competition seeks to make better predictions of runway throughputs using machine learning or other techniques. This competition engages students, faculty members, and other individuals employed by United States universities to develop a machine learning model that provides a short-term forecast of estimated airport runway throughput using simulated real-time information from historical NAS and weather forecast data, as well as other factors such as meteorological conditions, airport runway configuration, and airspace congestion.

Award: $120,000 in total prizes

Open Date: September 13, 2024

Close Date: December 8, 2024

For more information, visit: https://bitgrit.net/competition/23

4 Min Read NASA’s Artemis II Crew Uses Iceland Terrain for Lunar Training

Credits:
NASA/Trevor Graff/Robert Markowitz

Black and gray sediment stretches as far as the eye can see. Boulders sit on top of ground devoid of vegetation. Humans appear almost miniature in scale against a swath of shadowy mountains. At first glance, it seems a perfect scene from an excursion on the Moon’s surface … except the people are in hiking gear, not spacesuits.

Iceland has served as a lunar stand-in for training NASA astronauts since the days of the Apollo missions, and this summer the Artemis II crew took its place in that long history. NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen, along with their backups, NASA astronaut Andre Douglas and CSA astronaut Jenni Gibbons, joined geology experts for field training on the Nordic island.

NASA astronaut and Artemis II mission specialist Christina Koch stands in the desolate landscape of Iceland during a geology field training course. NASA/Robert Markowitz NASA/Robert Markowitz

“Apollo astronauts said Iceland was one of the most lunar-like training locations that they went to in their training,” said Cindy Evans, Artemis geology training lead at NASA’s Johnson Space Center in Houston. “It has lunar-like planetary processes – in this case, volcanism. It has the landscape; it looks like the Moon. And it has the scale of features astronauts will both be observing and exploring on the Moon.”

Iceland’s geology, like the Moon’s, includes rocks called basalts and breccias. Basalts are dark, fine-grained, iron-rich rocks that form when volcanic magma cools and crystalizes quickly. In Iceland, basalt lavas form from volcanoes and deep fissures. On the Moon, basalts can form from both volcanoes and lava pooling in impact basins. Breccias are angular fragments of rock that are fused together to create new rocks. In Iceland, volcanic breccias are formed from explosive volcanic eruptions and on the Moon, impact breccias are formed from meteoroids impacting the lunar surface.

Apollo astronauts said Iceland was one of the most lunar-like training locations that they went to in their training.

Cindy Evans

Artemis Geology Training Lead

Along with exploring the geology of Iceland, the astronauts practiced navigation and expeditionary skills to prepare them for living and working together, and gave feedback to instructors, who used this as an opportunity to hone their instruction and identify sites for future Artemis crew training. They also put tools to the test, learning to use hammers, scoops, and chisels to collect rock samples.

Caption: The Artemis II crew, NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and Canadian Space Agency (CSA) astronaut Jeremy Hansen, and backup crew members NASA astronaut Andre Douglas and CSA astronaut Jenni Gibbons trek across the Icelandic landscape during their field geology training. NASA/Robert Markowitz

“The tools we used during the Apollo missions haven’t changed that much for what we’re planning for the Artemis missions,” said Trevor Graff, exploration geologist and the hardware and testing lead on the Artemis science team at NASA Johnson. “Traditionally, a geologist goes out with just standard tool sets of things like rock hammers and scoops or shovels to sample the world around them, both on the surface and subsurface.”

The Artemis tools have a bit of a twist from traditional terrestrial geology tools, though. Engineers must take into consideration limited mass availability during launch, how easy it is to use a tool while wearing pressurized gloves, and how to ensure the pristine nature of the lunar samples is preserved for study back on Earth.

There’s really transformational science that we can learn by getting boots back on the Moon, getting samples back, and being able to do field geology with trained astronauts on the surface.

Angela Garcia

Exploration Geologist and Artemis II Science Officer

Caption: Angela Garcia, Artemis II science officer and exploration geologist, demonstrates how to use a rock hammer and chisel to dislodge a rock sample from a large boulder during the Artemis II field geology training in Iceland. NASA/Robert Markowitz

“There’s really transformational science that we can learn by getting boots back on the Moon, getting samples back, and being able to do field geology with trained astronauts on the surface,” said Angela Garcia, exploration geologist and an Artemis II science officer at NASA Johnson.

The Artemis II test flight will be NASA’s first mission with crew under Artemis and will pave the way to land the first woman, first person of color, and first international partner astronaut on the Moon on future missions. The crew will travel approximately 4,600 miles beyond the far side of the Moon. While the Artemis II astronauts will not land on the surface of the Moon, the geology fundamentals they develop during field training will be critical to meeting the science objectives of their mission.

These objectives include visually studying a list of surface features, such as craters, from orbit. Astronauts will snap photos of the features, and describe their color, reflectivity, and texture — details that can reveal their geologic history.

The Artemis II crew astronauts, their backups, and the geology training field team pose in a valley in Iceland’s Vatnajökull national park. From front left: Angela Garcia, Jacob Richardson, Cindy Evans, Jenni Gibbons, Jacki Mahaffey, back row from left: Jeremy Hansen, John Ramsey, Reid Wiseman, Ron Spencer, Scott Wray, Kelsey Young, Patrick Whelley, Christina Koch, Andre Douglas, Jacki Kagey, Victor Glover, Rick Rochelle (NOLS), Trevor Graff.

“Having humans hold the camera during a lunar pass and describe what they’re seeing in language that scientists can understand is a boon for science,” said Kelsey Young, lunar science lead for Artemis II and Artemis II science officer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “In large part, that’s what we’re training astronauts to do when we take them to these Moon-like environments on Earth.”

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node137893 GRGSantCristofol6GRGSantCristofol6 zonaLa Garriga posició (lat/lon)Lat:41.682458
Lon:2.2927320 metres des del terra disponible per fer xarxa i monitoritzarYesPlanned gràfics proveïts des deAgafar dels pares informació de contacte creat per: mdplus el 13/09/2024 - 2:48pm · actualitzat per: mdplus el Dv, 13/09/2024 - 15:01 trastos trastotipusipestatúltima disponibilitatunsolclic GRGSantCristofol6Rd1radio10.90.178.230/27PlannedRouterOSv6.x No estàs autoritzat a actualitzar aquest node. enllaços de xarxa (ap/client) nodes enllaçats (trastos)ipestatkms.az. GRGSantCristofol6Rd1 - LGarGRGSntCrstfl6Rd1CPE0 175085-GRG-WAIFAI-[56940] (GRG-WAIFAI-NORD)10.90.178.230/10.90.178.225Working0.742231-SO Total: 0.742 kms.

Hubble Space Telescope

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Hubble Examines a Spiral Star Factory This NASA/ESA Hubble Space Telescope image features the spiral galaxy NGC 5668. ESA/Hubble & NASA, C. Kilpatrick

This NASA/ESA Hubble Space Telescope image features a spiral galaxy in the constellation Virgo named NGC 5668. It is relatively near to us at 90 million light-years from Earth and quite accessible for astronomers to study with both space- and ground-based telescopes. At first glance, it doesn’t seem like a remarkable galaxy. It is around 90,000 light-years across, similar in size and mass to our own Milky Way galaxy, and its nearly face-on orientation shows open spiral arms made of cloudy, irregular patches.

One noticeable difference between the Milky Way galaxy and NGC 5668 is that this galaxy is forming new stars 60% more quickly. Astronomers have identified two main drivers of star formation in NGC 5668. Firstly, this high-quality Hubble view reveals a bar at the galaxy’s center, though it might look more like a slight oval shape than a real bar. The bar appears to have affected the galaxy’s star formation rate, as central bars do in many spiral galaxies. Secondly, astronomers tracked high-velocity clouds of hydrogen gas moving vertically between the disk of the galaxy and the spherical, faint halo which surrounds it. These movements may be the result of strong stellar winds from hot, massive stars, that would contribute gas to new star-forming regions.

The enhanced star formation rate in NGC 5668 comes with a corresponding abundance of supernova explosions. Astronomers have spotted three in the galaxy, in 1952, 1954, and 2004. In this image, Hubble examined the surroundings of the Type II SN 2004G, seeking to study the kinds of stars that end their lives as this kind of supernova.

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Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov

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Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center

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NASA's Europa Clipper is seen here on Aug. 21, 2024, in a clean room at the agency's Kennedy Space Center in Florida. The photo was taken as engineers and technicians deployed and tested the spacecraft's giant solar arrays, each of which measures about 46.5 feet (14.2 meters) long and about 13.5 feet (4.1 meters) high.

NASA/Frank Michaux

On Aug. 21, 2024, engineers and technicians deployed and tested NASA’s Europa Clipper giant solar arrays. Each array measures about 46.5 feet (14.2 meters) long and about 13.5 feet (4.1 meters) high.

Europa Clipper is scheduled to launch Oct. 10, 2024, on the first mission to conduct a detailed science investigation of Jupiter’s moon Europa. Scientists predict Europa has a salty ocean beneath its icy crust that could hold the building blocks necessary to sustain life.

Learn how this spacecraft’s solar arrays will power flybys.

Image credit: NASA/Frank Michaux

The International Space Station is pictured from the SpaceX Crew Dragon Endeavour during a fly around.NASA

NASA astronaut Nick Hague and Roscosmos cosmonaut Aleksandr Gorbunov are headed to the International Space Station for the agency’s SpaceX Crew-9 mission in September. Once on station, these crew members will support scientific investigations that include studies of blood clotting, effects of moisture on plants grown in space, and vision changes in astronauts.

Here are details on some of the work scheduled during the Crew-9 expedition:

Blood cell development in space

Megakaryocytes Orbiting in Outer Space and Near Earth (MeF1) investigates how environmental conditions affect the development and function of megakaryocytes and platelets. Megakaryocytes, large cells found in bone marrow, and platelets, pieces of these cells, play important roles in blood clotting and immune response.

“Understanding the development and function of megakaryocytes and platelets during long-duration spaceflight is crucial to safeguarding the health of astronauts,” said Hansjorg Schwertz, principal investigator, at the University of Utah. “Sending megakaryocyte cell cultures into space offers a unique opportunity to explore their intricate differentiation process. Microgravity also may impact other blood cells, so the insights we gain are likely to enhance our overall comprehension of how spaceflight influences blood cell production.”

Results could provide critical knowledge about the risks of changes in inflammation, immune responses, and clot formation in spaceflight and on the ground.

Scanning electron-microscopy image of human platelets prior to launch to the International Space Station.University of Utah/Megakaryocytes PI Team Patches for NICER

The Neutron Star Interior Composition Explorer (NICER) telescope on the exterior of the space station measures X-rays emitted by neutron stars and other cosmic objects to help answer questions about matter and gravity.

In May 2023, NICER developed a “light leak” that allows sunlight to interfere with daytime measurements. Special patches designed to cover some of the damage will be installed during a future spacewalk, returning the instrument to around-the-clock operation.

“This will be the fourth science observatory and first X-ray telescope in orbit to be repaired by astronauts,” said principal investigator Keith Gendreau at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “In just a year, we diagnosed the problem, designed and tested a solution, and delivered it for launch. The space station team — from managers and safety experts to engineers and astronauts — helped us make it happen. We’re looking forward to getting back to normal science operations.”

This view shows NICER’s 56 X-ray concentrators. Astronauts plan to cover some of them with special patches on a future spacewalk. NASA Vitamins for vision

Some astronauts experience vision changes, a condition called Spaceflight-Associated Neuro-ocular Syndrome. The B Complex investigation tests whether a daily B vitamin supplement can prevent or mitigate this problem and assesses how genetics may influence individual response.

“We still do not know exactly what causes this syndrome, and not everyone gets it,” said Sara Zwart, principal investigator, at the University of Texas Medical Branch, Houston. “It is likely many factors, and biological variations that make some astronauts more susceptible than others.”

One such variation could be related to a metabolic pathway that requires B vitamins to function properly. Inefficiencies in this pathway can affect the inner lining of blood vessels, resulting in leaks that may contribute to vision changes. Providing B vitamins known to affect blood vessel function positively could minimize issues in genetically at-risk astronauts.

“The concept of this study is based on 13 years of flight and ground research,” Zwart said. “We are excited to finally flight test a low-risk countermeasure that could mitigate the risk on future missions, including those to Mars.”

NASA astronaut Mark Vande Hei conducts a vision exam on the International Space StationNASA Watering the space garden

As people travel farther from Earth for longer, growing food becomes increasingly important. Scientists conducted many plant growth experiments on the space station using its Veggie hardware, including Veg-01B, which demonstrated that ‘Outredgeous’ red romaine lettuce is suitable for crop production in space.

Plant Habitat-07 uses this lettuce to examine how moisture conditions affect the nutritional quality and microbial safety of plants. The Advanced Plant Habitat controls humidity, temperature, air, light, and soil moisture, creating the precise conditions needed for the experiment.

Using a plant known to grow well in space removes a challenging variable from the equation, explained Chad Vanden Bosch, principal investigator at Redwire, and this lettuce also has been proven to be safe to consume when grown in space.

“For crews building a base on the Moon or Mars, tending to plants may be low on their list of responsibilities, so plant growth systems need to be automated,” Bosch said. “Such systems may not always provide the perfect growing conditions, though, so we need to know if plants grown in suboptimal conditions are safe to consume.”

This preflight image shows lettuce grown under control (left) and flood (right) moisture treatments. Plant Habitat-07 team

Melissa Gaskill

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node137892 SevaMontmany1SevaMontmany1 zonaSeva posició (lat/lon)Lat:41.839023
Lon:2.2859415 metres des del terra disponible per fer xarxa i monitoritzarYesPlanned gràfics proveïts des deAgafar dels pares informació de contacte creat per: setupinformatica.com el 12/09/2024 - 5:08pm Aquest node encara no te cap trasto No estàs autoritzat a actualitzar aquest node.

node137891 TonaCamSabellTonaCamSabell zonaTonaCami Sabell posició (lat/lon)Lat:41.859119
Lon:2.2354865 metres des del terra disponible per fer xarxa i monitoritzarYesWorking gràfics proveïts des deAgafar dels pares informació de contacte creat per: qrt el 12/09/2024 - 11:19am · actualitzat per: qrt el Dij, 12/09/2024 - 11:23 trastos trastotipusipestatúltima disponibilitatunsolclic TonaCamSabellRd1radio10.138.38.45/27WorkingRouterOSv6.x No estàs autoritzat a actualitzar aquest node. enllaços de xarxa (ap/client) nodes enllaçats (trastos)ipestatkms.az. TonaCamSabellRd1 - TonaTnCmSbllRd1CPE0 175082-TonaCastell-[2231] (TonaCastellST/TonaCastellAP5)10.138.38.45/10.138.38.33Planned1.072237-SO Total: 1.072 kms.

node137890 CSOPrieresXXPrieres, XX zonaCaso (municipio)Caso posició (lat/lon)Lat:43.214432
Lon:-5.3751315 metres des del terra disponible per fer xarxa i monitoritzarYesPlanned gràfics proveïts des deAgafar dels pares informació de contacte creat per: sestaferia.net el 12/09/2024 - 11:04am Aquest node encara no te cap trasto No estàs autoritzat a actualitzar aquest node.

node137889 TonaCam4CTonaCam4C zonaTona4 Carreteres posició (lat/lon)Lat:41.845267
Lon:2.2317345 metres des del terra disponible per fer xarxa i monitoritzarYesWorking gràfics proveïts des deAgafar dels pares informació de contacte creat per: qrt el 12/09/2024 - 10:35am · actualitzat per: qrt el Dij, 12/09/2024 - 10:39 trastos trastotipusipestatúltima disponibilitatunsolclic TonaCam4CRd1radio10.139.163.242/24WorkingRouterOSv6.x No estàs autoritzat a actualitzar aquest node. enllaços de xarxa (ap/client) nodes enllaçats (trastos)ipestatkms.az. TonaCam4CRd1 - TonaTnCm4CRd1CPE0 175081-TonaCastell-[2231] (TonaCastellST/TonaCastellAP5)10.139.163.242/10.139.163.1Planned1.126328-NO Total: 1.126 kms.

node137888 CiSLesOliveresCiSLesOliveres zonaCànoves i Samalús posició (lat/lon)Lat:41.688491
Lon:2.3191880 metres des del terra disponible per fer xarxa i monitoritzarYesPlanned gràfics proveïts des deAgafar dels pares informació de contacte creat per: mdplus el 12/09/2024 - 8:36am Aquest node encara no te cap trasto No estàs autoritzat a actualitzar aquest node.

Chile pepper plants growing in the Advanced Plant Habitat aboard the International Space Station bore fruit in the late summer and fall of 2021. Overcoming the challenges of growing fruit in microgravity is important to NASA for long-duration missions during which crew members will need good sources of Vitamin C to supplement their diets.