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By NASA
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s ECOSTRESS instrument on June 19 recorded scorching roads and sidewalks across Phoenix where contact with skin could cause serious burns in minutes to seconds, as indicated in the legend above. NASA/JPL-Caltech Roads and sidewalks in some areas get so hot that skin contact could result in second-degree burns.
Researchers at NASA’s Jet Propulsion Laboratory in Southern California have mapped scorching pavement in Phoenix where contact with skin — from a fall, for example — can cause serious burns. The image shows land surface temperatures across a grid of roads and adjacent sidewalks, revealing how urban spaces can turn hazardous during hot weather.
Data for this visualization of the Phoenix area — the fifth most populous city in the United States — was collected at 1:02 p.m. local time on June 19, 2024, by a NASA instrument aboard the International Space Station. Called ECOSTRESS (short for the Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station), the instrument measures thermal infrared emissions from Earth’s surface.
The Image shows how miles of asphalt and concrete surfaces (colored here in yellow, red, and purple, based on temperature) trap heat. The surfaces registered at least 120 degrees Fahrenheit (49 degrees Celsius) to the touch — hot enough to cause contact burns in minutes to seconds.
The image also shows cooling effects of green spaces in communities like Encanto and Camelback East, in contrast to the hotter surface temperatures seen in Maryvale and Central City, where there are fewer parks and trees.
“We create these maps to be intuitive to users and help make data more accessible to the public and citizens scientists,” said Glynn Hulley, a JPL climate researcher. “We see them as a vital tool for planning effective heat interventions, such as tree planting, that can cool down the hottest roads and sidewalks.”
Homing in on Heat
At the lower right of the image is Phoenix’s Sky Harbor International Airport, where ECOSTRESS recorded some of the hottest land surface temperatures within the city —around 140 F (60 C). The air temperature on June 19 at the airport reached 106 F (43 C).
Air temperature, which is measured out of direct sunlight, can differ significantly from the temperature at the land surface. Streets are often the hottest surfaces of the built environment due to dark asphalt paving that absorbs more sunlight than lighter-colored surfaces; asphalt absorbs up to 95% of solar radiation. These types of surfaces can easily be 40 to 60 degrees F (22 to 33 degrees C) hotter than the air temperature on a very hot day.
Launched to the International Space Station in 2018, ECOSTRESS has as its primary mission the identification of plants’ thresholds for water use and water stress, giving insight into their ability to adapt to a warming climate. But the instrument is also useful for documenting other heat-related phenomena, like patterns of heat absorption and retention.
To produce the image of Phoenix, scientists used a machine learning algorithm that incorporates data from additional satellites: NASA/USGS Landsat and Sentinel-2. The combined measurements were used to “sharpen” the surface temperatures to a resolution of 100 feet (30 meters) by 100 feet (30 meters).
More About the Mission
JPL built and manages the ECOSTRESS mission for the Earth Science Division in the Science Mission Directorate at NASA Headquarters in Washington. ECOSTRESS is an Earth Venture Instrument mission; the program is managed by NASA’s Earth System Science Pathfinder program at NASA’s Langley Research Center in Hampton, Virginia.
More information about ECOSTRESS is available here: https://ecostress.jpl.nasa.gov/.
News Media Contacts
Jane J. Lee / Andrew Wang
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0307 / 626-379-6874
jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov
Written by Sally Younger
2024-096
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Last Updated Jul 02, 2024 Related Terms
Ecostress (ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station) Earth Science Extreme Weather Events Jet Propulsion Laboratory Weather and Atmospheric Dynamics Explore More
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By NASA
ASIA-AQ DC-8 aircraft flies over Bangkok, Thailand to monitor seasonal haze from fire smoke and urban pollution. Photo credit: Rafael Luis Méndez Peña. Tracking the spread of harmful air pollutants across large regions requires aircraft, satellites, and diverse team of scientists. NASA’s global interest in the threat of air pollution extends into Asia, where it works with partners on the Airborne and Satellite Investigation of Asian Air Quality (ASIA-AQ). This international mission integrates satellite data and aircraft measurements with local air quality ground monitoring and modeling efforts across Asia.
Orchestrating a mission of this scale requires complicated agreements between countries, the coordination of aircraft and scientific instrumentation, and the mobilization of scientists from across the globe. To make this possible, ARC’s Earth Science Project Office (ESPO) facilitated each phase of the campaign, from site preparation and aircraft deployment to sensitive data management and public outreach.
“Successfully meeting the ASIA-AQ mission logistics requirements was an incredible effort in an uncertainty-filled environment and a very constrained schedule to execute and meet those requirements,” explains ASIA-AQ Project Manager Jhony Zavaleta. “Such effort drew on the years long experience on international shipping expertise, heavy equipment operations, networking and close coordination with international service providers and all of the U.S. embassies at each of our basing locations.”
Map of planned ASIA-AQ operational regions. Yellow circles indicate the original areas of interest for flight sampling. The overlaid colormap shows annual average nitrogen dioxide (NO2) concentrations observed by the TROPOMI satellite with red colors indicating the most polluted locations. Understanding Air Quality Globally
ASIA-AQ benefits our understanding of air quality and the factors controlling its daily variability by investigating the ways that air quality can be observed and quantified. The airborne measurements collected during the campaign are directly integrated with existing satellite observations of air quality, local air quality monitoring networks, other available ground assets, and models to provide a level of detail otherwise unavailable to advance understanding of regional air quality and improve future integration of satellite and ground monitoring information.
ESPO’s Mission-Critical Contributions
Facilitating collaboration between governmental agencies and the academic community by executing project plans, navigating bureaucratic hurdles, and consensus building. Mission planning for two NASA aircraft. AFRC DC-8 completed 16 science flights, totaling 125 flight hours. The LaRC GIII completed 35 science flights, totaling 157.7 flight hours. Enabling international fieldwork and workforce mobilization by coordinating travel, securing authorizations and documentation, and maintaining relationships with local research partners. Managing outreach to local governments and schools. ASIA-AQ team members showcased tools used for air quality science to elementary/middle/high school students. Recent news feature here. View of ASIA-AQ aircraft in Bangkok, Thailand. ESPO staff from left to right: Dan Chirica, Marilyn Vasques, Sam Kim, Jhony Zavaleta, and Andrian Liem. Aircraft from left to right: Korean Meteorological Agency/National Institute of Meteorological Sciences, NASA LaRC GIII, NSASA DC-8, (2) Hanseo University, Sunny Air (private aircraft contracted by Korean Meteorological Agency). Photo: Rafael Mendez Peña. The flying laboratory of NASA’s DC-8
NASA flew its DC-8 aircraft, picture above, equipped with instrumentation to monitor the quality, source, and movement of harmful air pollutants. Scientists onboard used the space as a laboratory to analyze data in real-time and share it with a network of researchers who aim to tackle this global issue.
“Bringing the DC-8 flying laboratory and US researchers to Asian countries not only advances atmospheric research but also fosters international scientific collaboration and education,” said ESPO Project Specialist Vidal Salazar. “Running a campaign like ASIA AQ also opens doors for shared knowledge and exposes local communities to cutting-edge research.”
Fostering Partnerships Through Expertise and Goodwill
International collaboration fostered through this campaign contributes to an ongoing dialogue about air pollution between Asian countries.
“NASA’s continued scientific and educational activities around the world are fundamental to building relationships with partnering countries,” said ESPO Director Marilyn Vasques. “NASA’s willingness to share data and provide educational opportunities to locals creates goodwill worldwide.”
The role of ESPO in identifying, strategizing, and executing on project plans across the globe created a path for multi-sectoral community engagement on air quality. These global efforts to improve air quality science directly inform efforts to save lives from this hazard that affects all.
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By European Space Agency
Video: 00:03:29 Mars’s surface is covered in all manner of scratches and scars. Its many marks include the fingernail scratches of Tantalus Fossae, the colossal canyon system of Valles Marineris, the oddly orderly ridges of Angustus Labyrinthus, and the fascinating features captured in today’s video release from Mars Express: the cat scratches of Nili Fossae.
Nili Fossae comprises parallel trenches hundreds of metres deep and several hundred kilometres long, stretching out along the eastern edge of a massive impact crater named Isidis Planitia.
This new video features observations from Mars Express's High Resolution Stereo Camera (HRSC). It first flies northwards towards and around these large trenches, showing their fractured, uneven appearance, before turning back to head southwards. It ends by zooming out to a ‘bird’s eye’ view, with the landing site of NASA’s Perseverance rover, Jezero Crater, visible in the lower-middle part of the final scene. (You can explore this crater further via ESA’s interactive map.)
The trenches of Nili Fossae are actually features known as ‘graben’, which form when the ground sitting between two parallel faults fractures and falls away. As the graben seem to curve around Isidis Planitia, it’s likely that they formed as Mars’s crust settled following the formation of the crater by an incoming space rock hitting the surface. Similar ruptures – the counterpart to Nili Fossae – are found on the other side of the crater, and named Amenthes Fossae.
Scientists have focused on Nili Fossae in recent years due to the impressive amount and diversity of minerals found in this area, including silicates, carbonates, and clays (many of which were discovered by Mars Express’s OMEGA instrument). These minerals form in the presence of water, indicating that this region was very wet in ancient martian history. Much of the ground here formed over 3.5 billion years ago, when surface water was abundant across Mars. Scientists believe that water flowed not only across the surface here but also beneath it, forming underground hydrothermal flows that were heated by ancient volcanoes.
Because of what it could tell us about Mars’s ancient and water-rich past, Nili Fossae was considered as a possible landing site for NASA’s Curiosity rover, before the rover was ultimately sent to Gale Crater in 2012. Another mission, NASA’s Perseverance rover, was later sent to land in the nearby Jezero Crater, visible at the end of this video.
Mars Express has visited Nili Fossae before, imaging the region’s graben system back in 2014. The mission has orbited the Red Planet since 2003, imaging Mars’s surface, mapping its minerals, studying its tenuous atmosphere, probing beneath its crust, and exploring how various phenomena interact in the martian environment. For more from the orbiter and its HRSC, see ESA's Mars Express releases.
Disclaimer: This video is not representative of how Mars Express flies over the surface of Mars. See processing notes below.
Processing notes: The video is centred at 23°N, 78°E. It was created using Mars Chart (HMC30) data, an image mosaic made from single-orbit observations from Mars Express’s HRSC. This mosaic was combined with topography derived from a digital terrain model of Mars to generate a three-dimensional landscape. For every second of the movie, 62.5 separate frames are rendered following a pre-defined camera path. The vertical exaggeration is three-fold. Atmospheric effects – clouds and haze – have been added, and start building up at a distance of 50 km.
Click here for the original video created by Freie Universität Berlin, who use Mars Express data to prepare spectacular views of the martian surface. The original version has no voiceover, captions or ESA logo.
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By NASA
These images represent a sample of galaxy clusters that are part of the largest and most complete study to learn what triggers stars to form in the universe’s biggest galaxies. Clusters of galaxies are the largest objects in the universe held together by gravity and contain huge amounts of hot gas seen in X-rays. This research, made using Chandra and other telescopes, showed that the conditions for stellar conception in these exceptionally massive galaxies have not changed over the last ten billion years. In these images, X-rays from Chandra are shown along with optical data from Hubble.X-ray: NASA/CXC/MIT/M. Calzadilla el al.; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/N. Wolk & J. Major These four images represent a sample of galaxy clusters that are part of the largest and most complete study to learn what triggers stars to form in the universe’s biggest galaxies, as described in our latest press release. This research, made using NASA’s Chandra X-ray Observatory and other telescopes, showed that the conditions for stellar conception in these exceptionally massive galaxies have not changed over the last ten billion years.
Galaxy clusters are the largest objects in the universe held together by gravity and contain huge amounts of hot gas seen in X-rays. This hot gas weighs several times the total mass of all the stars in all the hundreds of galaxies typically found in galaxy clusters. In the four galaxy cluster images in this graphic, X-rays from hot gas detected by Chandra are in purple and optical data from NASA’s Hubble Space Telescope, mostly showing galaxies in the clusters, are yellow and cyan.
In this study, researchers looked at the brightest and most massive class of galaxies in the universe, called brightest cluster galaxies (BCGs), in the centers of 95 clusters of galaxies. The galaxy clusters chosen are themselves an extreme sample — the most massive clusters in a large survey using the South Pole Telescope (SPT), with funding support from the National Science Foundation and Department of Energy — and are located between 3.4 and 9.9 billion light-years from Earth.
The four galaxy clusters shown here at located at distances of 3.9 billion (SPT-CLJ0106-5943), 5.6 billion (SPT-CLJ0307-6225), 6.4 billion (SPT-CLJ0310-4647) and 7.7 billion (SPT-CLJ0615-5746) light-years from Earth, and the images are 1.7 million, 2 million, 2.4 million and 2.2 million light-years across, respectively. By comparison our galaxy is only about 100,000 light-years across.
In SPT-CLJ0307-6225 the BCG is near the bottom right of the image and in the other images they are near the centers. Some of the long, narrow features are caused by gravitational lensing, where mass in the clusters is warping the light from galaxies behind the clusters. The images have been rotated from standard astronomer’s configuration of North up by 20 degrees clockwise (SPT-CLJ0106-5943), 6.2 degrees counterclockwise (SPT-CLJ0307-6225), 29,2 degrees counterclockwise (SPT-CLJ0310-4647) and 24.2 degrees clockwise (SPT-CLJ0615-5746).
The team found that the precise trigger for stars to form in the galaxies that they studied is when the amount of disordered motion in the hot gas — a physical concept called “entropy” — falls below a critical threshold. Below this threshold, the hot gas inevitably cools to form new stars.
In addition to the X-ray data from Chandra X-ray Observatory and radio data from the SPT already mentioned, this result also used radio data from the Australia Telescope Compact Array, and the Australian SKA Pathfinder Telescope, infrared data from NASA’s WISE satellite, and several optical telescopes. The optical telescopes used in this study were the Magellan 6.5-m Telescopes, the Gemini South Telescope, the Blanco 4-m Telescope (DECam, MOSAIC-II) and the Swope 1m Telescope. A total of almost 50 days of Chandra observing time was used for this result.
Michael Caldazilla of the Massachusetts Institute of Technology (MIT) presented these results at the 243rd meeting of the American Astronomical Society in New Orleans, LA. In addition, there is a paper submitted to The Astrophysical Journal led by Caldazilla on this result (preprint here). The other authors on the paper are Michael McDonald (MIT), Bradford Benson (University of Chicago), Lindsay Bleem (Argonne National Laboratory), Judith Croston (The Open University, UK), Megan Donahue (Michigan State University), Alastair Edge (University of Durham, UK), Gordon Garmire (Penn State University), Julie Hvalacek-Larrondo (University of Colorado), Minh Huynh (CSIRO, Australia), Gourav Khullar (University of Pittsburgh), Ralph Kraft (Center for Astrophysics | Harvard & Smithsonian), Brian McNamara (University of Waterloo, Canada), Allison Noble (Arizona State University), Charles Romero (CfA), Florian Ruppin (University of Lyon, France), Taweewat Somboonpanyakul (Stanford University), and Mark Voit (Michigan State).
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Read more from NASA’s Chandra X-ray Observatory.
For more Chandra images, multimedia and related materials, visit:
https://www.nasa.gov/mission/chandra-x-ray-observatory/
Visual Description
This release includes composite images of four galaxy clusters, presented in a two-by-two grid. Each image features a hazy, purple cloud representing X-rays from hot gas observed by Chandra. The distant galaxies in and around the clouds of hot gas have been captured in optical data, and are shown in golden yellows with hints of vibrant cyan blue.
The galaxy cluster at our upper left is labeled SPT-CLJ0310-4647. Here, the blackness of space is packed with gleaming specks of white, golden yellow, and bright blue light. These are individual galaxies. Some of the galaxies resemble blurred, glowing dots. In other galaxies, the curving arms of a spiral formation are discernible. At the center of the image, a faint purple cloud surrounds several of the cluster’s brightest galaxies.
At our upper right is an image of SPT-CLJ0615-5746. This is the most distant cluster of the four so the galaxies it contains appear relatively small. These galaxies are mostly located near the center of the image. The purple cloud of hot gas is roughly spherical, and has a light purple spot at its core.
At our lower right is SPT-CLJ0307-6225. Here, X-rays from hot gas are represented by a large, misty, purple cloud that covers much of the image. The brightest spot in the cloud is a light purple dot near our lower right. The most notable galaxy in this image is a pixilated spiral galaxy above and to our left of center.
The galaxy cluster at our lower left is labeled SPT-CLJ0106-5943. This cluster features a scattering of cyan blue galaxies, several of which appear stretched or elongated due to gravitational lensing. At the center of the image is a purple gas cloud with a bright white speck at its core.
News Media Contact
Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
Jonathan Deal
Marshall Space Flight Center
Huntsville, Ala.
256-544-0034
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By NASA
NASA Administrator Bill Nelson gives remarks after Indian Ambassador to the United States Taranjit Sandhu signed the Artemis Accords, Wednesday, June 21, 2023, at the Willard InterContinental Hotel in Washington.NASA/Bill Ingalls NASA Administrator Bill Nelson will travel to India and the United Arab Emirates (UAE) for a series of meetings beginning Monday, Nov. 27, with key government officials.
Nelson also will meet with space officials in both countries to deepen bilateral cooperation across a broad range of innovation and research-related areas, especially in human exploration and Earth science.
The visit to India fulfills a commitment through the United States and India initiative on Critical and Emerging Technology spearheaded by President Joe Biden. Nelson will visit several locations in India, including the Bengaluru-based facilities where the NISAR spacecraft, a joint Earth-observing mission between NASA and the Indian Space Research Organization (ISRO), is undergoing testing and integration for launch in 2024. NISAR is short for NASA ISRO Synthetic Aperture Radar.
As the first satellite mission between NASA and ISRO, NISAR is a revolutionary Earth-observing instrument, the first in the Earth System Observatory, that will measure Earth’s changing ecosystems, dynamic surfaces, and ice masses providing information about biomass, natural hazards, sea level rise, and groundwater, key information to guide efforts related to climate change, hazard mitigation, agriculture, and more.
While in the UAE, Nelson will participate in the 2023 United Nations Climate Change Conference, highlighting NASA’s role as a global leader in providing decisionmakers with critical Earth-science data. It will be the first time a NASA administrator will have attended the conference.
Students in each country also will have the opportunity to meet with Nelson to discuss science, technology, engineering, and mathematics (STEM) education and their roles as members of the Artemis Generation.
For more information about NASA’s international partnerships, visit:
https://www.nasa.gov/oiir
-end-
Jackie McGuinness
Headquarters, Washington
202-358-1600
jackie.mcguinness@nasa.gov
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Last Updated Nov 24, 2023 Location NASA Headquarters Related Terms
Missions NISAR (NASA-ISRO Synthetic Aperture Radar) View the full article
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