lundi 9 janvier 2023

Hubble Gazes at Colorful Cluster of Scattered Stars

 







NASA / ESA - Hubble Space Telescope (HST) patch.


Jan 9, 2023

The scattered stars of the globular cluster NGC 6355 are strewn across this image from the NASA/ESA Hubble Space Telescope. NGC 6355 is a galactic globular cluster that resides in our Milky Way galaxy's inner regions. It is less than 50,000 light-years from Earth in the constellation Ophiuchus.

Globular clusters are stable, tightly bound groups of tens of thousands to millions of stars that are associated with all types of galaxies. Their dense populations of stars and mutual gravitational attraction give these clusters a roughly spherical shape that holds a bright, central concentration of stars surrounded by an increasingly sparse sprinkling of stars. The dense, bright core of NGC 6355 shines in crystal-clear detail as Hubble is able to resolve individual stars in the crowded area toward the center of this image.

Hubble has revolutionized the study of globular clusters. It is almost impossible to distinguish individual stars in globular clusters with ground-based telescopes. Hubble’s unique capabilities and vantage point above Earth’s light-distorting atmosphere allow it to capture a globular cluster’s constituent stars in detail. This image contains data from Hubble’s Advanced Camera for Surveys and Wide Field Camera 3.

Hubble Space Telescope (HST)

For more information about Hubble, visit:

http://hubblesite.org/

http://www.nasa.gov/hubble

https://esahubble.org/

Related links:

Advanced Camera for Surveys: https://www.nasa.gov/content/hubble-space-telescope-advanced-camera-for-surveys

Wide Field Camera 3: https://www.nasa.gov/content/hubble-space-telescope-wide-field-camera-3

Text Credits: European Space Agency (ESA)/NASA/Andrea Gianopoulos/Image, Animation Credits: ESA/Hubble & NASA, E. Noyola, R. Cohen.

Best regards, Orbiter.ch

NASA Space Missions Pinpoint Sources of CO2 Emissions on Earth

 






NASA - OCO-2 & OCO-3 Missions patch.


Jan 9, 2023

A case study involving Europe’s largest coal-fired power plant shows space-based observations can be used to track carbon dioxide emissions – and reductions – at the source.

Image above: Lights brighten the night sky in this image of Europe, including Poland, taken from the International Space Station. Aboard the orbiting laboratory is NASA’s OCO-3, an instrument that can be used for tracking carbon dioxide emission changes at a local scale. Image Credit: NASA.

A duo of Earth-observing missions has enabled researchers to detect and track carbon dioxide (CO2) emission changes from a single facility, using the world’s fifth-largest coal-fired power plant as a test case.

In the recent study, researchers used space-based measurements from NASA’s Orbiting Carbon Observatory (OCO) 2 and 3 missions to quantify the carbon dioxide discharged hundreds of miles below at Bełchatów Power Station in Poland, the largest single emitter in Europe. Analyzing the plant’s emission plumes from several satellite overpasses between 2017 and 2022, they detected changes in carbon dioxide levels that were consistent with hourly fluctuations in electricity generation. Temporary and permanent unit shutdowns (for maintenance or decommissioning) reduced the plant’s overall emissions, which the team was able to detect as well.

The findings demonstrate that space-based observations can be used to track carbon dioxide emission changes at a local scale, the scientists said.

Image above: This illustration shows NASA’s OCO-2 satellite, launched in 2014. As it orbits Earth, the spacecraft maps natural and human-made carbon dioxide emissions on scales ranging from regions to continents. Light-analyzing spectrometers are tuned to detect the telltale signature of the gas. Image Credits: NASA/JPL-Caltech.

Launched in 2014, NASA’s OCO-2 satellite maps natural and human-made (anthropogenic) carbon dioxide emissions on scales ranging from regions to continents. The instrument samples the gas indirectly by measuring the intensity of sunlight reflected off Earth’s surface and absorbed by carbon dioxide in the column of air from the ground to the satellite. OCO-2’s spectrometers are tuned to detect the specific signature of CO2 gas.

Spare components from that mission were used to create OCO-3, an instrument that has flown on the International Space Station since 2019. OCO-3 was designed with a mapping mode that can make multiple sweeping observations as the space station passes over an area, allowing researchers to create detailed mini-maps from a city-scale area of interest.

Neither OCO instrument was originally designed specifically to detect emissions from individual facilities such as Bełchatów, so the new findings are a “pleasant surprise,” said Abhishek Chatterjee, project scientist for the OCO-3 mission at NASA’s Jet Propulsion Laboratory in Southern California. “As a community we are refining the tools and techniques to be able to extract more information from the data than what we had originally planned,” he added. “We are learning that we can actually understand a lot more about anthropogenic emissions than what we had previously expected.”

Image above: This illustration shows NASA’s OCO-3 mounted on the underside of the International Space Station. The instrument, launched in 2019, was not originally designed to detect carbon dioxide emissions from individual facilities but scientists said it will be used for more point-source studies in the future. Image Credits: NASA/JPL-Caltech.

Tracking Carbon Into the Future

Emissions from large facilities such as power plants and refineries account for about half of global carbon dioxide emissions from fossil fuels. Bełchatów Power Station, in operation since 1988, is the largest lignite-fired power plant in the world, with a reported capacity of 5,102 megawatts. Lignite (brown coal) typically leads to higher emissions per megawatt generated than anthracite (hard coal). The Polish government has drafted plans to close the plant by the end of 2036.

Ray Nassar, a senior researcher at Environment and Climate Change Canada and the study’s lead author, noted that most carbon dioxide emissions reports are created from estimates or data collected at the land surface. Researchers account for the mass of fossil fuels purchased and used, then calculate the expected emissions; they generally do not make actual atmospheric carbon dioxide measurements.

“The finer details about exactly when and where emissions occur are often not available,” Nassar said. “Providing a more detailed picture of carbon dioxide emissions could help to track the effectiveness of policies to reduce emissions. Our approach with OCO-2 and OCO-3 can be applied to more power plants or modified for carbon dioxide emissions from cities or countries.”

Because of the mapping mode observations of OCO-3, NASA data could be used more extensively in quantifying CO2 point-source emissions in the future. NASA recently announced that mission operations will be extended for several more years aboard the space station, and the instrument will operate alongside another greenhouse gas observer aboard the space station, the Earth Surface Mineral Dust Source Investigation (EMIT).

“It is really exciting to think that we will get another five to six years of operations with OCO-3,” Chatterjee said. “We are seeing that making measurements at the right time and at the right scale is critical.”

He added that OCO-3 can serve as a “pathfinder” for next-generation satellite missions. The OCO-2 and OCO-3 projects are managed by JPL. Caltech manages JPL for NASA.

Related links:

Space-based measurements from NASA’s Orbiting Carbon Observatory (OCO) 2 and 3 missions study: 

https://doi.org/10.3389/frsen.2022.1028240

OCO-2 (Orbiting Carbon Observatory 2): http://www.nasa.gov/mission_pages/oco2/index.html

OCO-3 (Orbiting Climate Observatory 3): https://www.nasa.gov/mission_pages/oco3/index.html

Images (mentioned), Text, Credits: NASA/Tony Greicius/JPL/Jane J. Lee/Andrew Wang/Written by Sally Younger.

Greetings, Orbiter.ch

Sentinel-1 and AI uncover glacier crevasses

 





ESA - Sentinel-1 Mission logo.


Jan 9, 2023

Scientists have developed a new Artificial Intelligence, or AI, technique using radar images from Europe’s Copernicus Sentinel-1 satellite mission, to reveal how the Thwaites Glacier Ice Tongue in West Antarctica is being damaged by squeezing and stretching as it flows from the middle of the continent to the coast. Being able to track fractures and crevasses in the ice beneath the overlying snow is key to better predicting the fate of floating ice tongues under climate change.

Thwaites Glacier

A paper published today in Nature Geoscience describes how ESA’s development of the Copernicus Sentinel-1 satellites and routine synthetic aperture radar imaging of coastal Antarctica coupled with a novel artificial intelligence algorithm, has provided a glaciology tool with forensic science capability.

The paper’s authors – a team of scientists from the University of Leeds and the University of Bristol in the UK – developed an AI algorithm, originally used to identify cells in microscope images, to spot crevasses forming in the ice in Sentinel-1’s radar images of Thwaites Glacier Ice Tongue, as shown in the animation below.

Crevasses, or cracks opening in the moving ice mass, are indicators of stresses building up in the glacier.

Thwaites’ crevasses in motion

Thwaites is a particularly important part of the Antarctic Ice Sheet because it holds enough ice to raise global sea levels by around 60 cm and is considered by many to be at risk of rapid retreat, threatening coastal communities around the world.

This new use of artificial intelligence will allow scientists to more accurately monitor and model changes to this important glacier.

The research focused on a part of the glacier system where the ice flows into the sea and begins to float – a point known as the grounding line. It forms the start of the Thwaites Eastern Ice Shelf and the western Thwaites Glacier Ice Tongue, which is also an ice shelf.

Thwaites Ice Tongue from Sentinel-2

Despite being small in comparison to the size of the entire glacier, changes to the ice shelves could have wide-ranging implications for the whole glacier system and future sea-level rise.

The scientists wanted to know if crevassing or fracture formation in the glacier was more likely to occur with changes to the speed of the ice flow.

Using machine learning, the researchers taught a computer to look at radar images from the Copernicus Sentinel-1 mission and identify changes over the last decade.

Sentinel-1’s all-weather radar allows scientists to track ice movement and peer through snow cover to unveil Thwaites Glacier Tongue’s crocodile skin-like appearance, which is normally hidden from sight.

Sentinel-1 - Radar vision

The analysis revealed that over the last six years, the Thwaites Glacier Ice Tongue has sped up and slowed down twice, by around 40% each time – from 4 km a year to 6 km a year before slowing. This is a substantial increase in the magnitude and frequency of speed change compared with past records.

The study found a complex interplay between crevasse formation and speed of the ice flow. When the ice flow quickens or slows, more crevasses are likely to form. In turn, the increase in crevasses causes the ice to change speed as the friction between the ice and underlying rock alters. 

Dr Anna Hogg, a glaciologist at the University of Leeds, said, “Dynamic changes on ice shelves are traditionally thought to occur on timescales of decades to centuries, so it was surprising to see this huge glacier speed up and slow down so quickly.  

“The study also demonstrates the key role that fractures play in un-corking the flow of ice, a process known as unbuttressing. 

“Ice-sheet models must be evolved to account for the fact that ice can fracture, which will allow us to measure future sea-level contributions more accurately.”

Thwaites flow

Trystan Surawy-Stepney, lead author of the paper and a doctoral researcher at the University of Leeds, added, “The nice thing about this study is the precision with which the crevasses were mapped. 

“It has been known for a while that crevassing is an important component of ice-shelf dynamics and this study demonstrates that this link can be studied on a large scale with beautiful resolution, using computer vision techniques applied to the deluge of satellite images acquired each week.”

Satellites orbiting Earth provide scientists with new data over the most remote and inaccessible regions of Antarctica. The radar on Sentinel-1 allows places like Thwaites Glacier to be imaged day or night, every week, all year round.

Thwaites and Pine Island Glaciers in West Antarctica

ESA’s Dr Mark Drinkwater commented, “Studies like this would not be possible without the large volume of high-resolution Antarctic ice-sheet image data provided by Sentinel-1.

“By continuing to plan and prepare future polar-orbiting missions, we can carry on supporting work like this and broaden the scope of scientific research on vital areas of Earth’s climate system.” 

As for the Thwaites Glacier Ice Tongue, it remains to be seen whether such short-term changes have any impact on the long-term dynamics of the glacier, or whether they are simply isolated symptoms of an ice shelf close to its end.

Related links:

Nature Geoscience: https://www.nature.com/articles/s41561-022-01097-9

Sentinel-1: https://www.esa.int/Applications/Observing_the_Earth/Copernicus/Sentinel-1

Images, Animation, Video, Text, Credits: ESA/Contains modified Copernicus Sentinel data (2019), processed by ESA, CC BY-SA 3.0 IGO/Contains modified Copernicus Sentinel data (2016–2021), processed by the University of Leeds and ESA/ATG medialab.

Best regards, Orbiter.ch

Galactic Energy - Ceres-1 launches five satellites

 







Galactic Energy - Ceres-1 / "Give Me Five" Mission patch.


Jan 9, 2023

Ceres-1 carrying five satellites liftoff

A Ceres-1 launch vehicle (Y5) launched five satellites from the Jiuquan Satellite Launch Center, Gansu Province, China, on 9 January 2023, at 05:04 UTC (13:04 local time).

Ceres-1 launches five satellites

Ceres-1 (谷神星一号) is a small solid propellant launch vehicle developed by Galactic Energy (星河动力) to carry a payload of up to 350 kg to low Earth orbit (LEO). According to official sources, the satellites were successfully placed into the planned orbits and will be used for commercial remote sensing, meteorological observations and Internet services.

Galactic Energy: https://www.galactic-energy.cn/index.php/En

Image, Video, Text, Credits: Galactic Energy/China Central Television (CCTV)/SciNews/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

CASC - Long March-7A launches Shijian-23, Shiyan-22A and Shiyan-22B

 







CASC - CZ-7A WSLS / Long March-7A / Shiyan-22A, 22B, 23 patch.


Jan 9, 2023

Long March-7A carrying Shijian-23, Shiyan-22A and Shiyan-22B liftoff

A Long March-7A launch vehicle (Y4) launched three satellites, Shijian-23, Shiyan-22A and Shiyan-22B, from the Wenchang Spacecraft Launch Site Hainan Province, China, on 8 January 2023, at 22:00 UTC (9 January, at 06:00 local time).

Long March-7A launches Shijian-23, Shiyan-22A and Shiyan-22B

According to official sources, the satellites entered their planned orbits successfully. Shijian-23 (实践二十三) will be “mainly used for scientific experiments and technical verification”. Shiyan-22A and Shiyan-22B will be used for “in-orbit verification tests of new technologies, such as space environment monitoring”.

For more information about China Aerospace Science and Technology Corporation (CASC), visit: http://english.spacechina.com/n16421/index.html

Image, Video, Text, Credits: China Central Television (CCTV)/China Aerospace Science and Technology Corporation (CASC)/SciNews/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

China’s Tianwen-1 Mars orbiter and rover appear to be in trouble

 







CNSA - Tianwen-1 (天問-1) Mission to Mars logo.


Jan 9, 2023

The two spacecraft making up China’s first interplanetary mission are both suffering issues, with the rover potentially lost on the surface after winter hibernation.

The Zhurong Mars rover has been hibernating on the Martian surface since May 18 last year and was expected to resume activity in December, around the time of the Spring equinox in the northern hemisphere.

Image above: China's Zhurong images its own parachute from a distance of 30 meters, July 12, 2021. Image Credits: CNSA/PEC.

However no announcement of establishing contact with the rover has been made. The South China Morning Post reported Jan. 7, citing sources that do not wish to be named, that teams on Earth have yet to receive a signal from Zhurong.

The Zhurong rover landed in Mars’s Utopia Planitia region in May 2021 but entered a period of hibernation to ride out winter, when both temperatures and solar radiation levels are too low for the solar-powered rover to operate.

The rover was expected to autonomously resume activities once it can generate sufficient energy from solar power and when temperatures reach around minus 15 degrees Celsius.

Zhurong entered hibernation when local temperatures were around minus 20 degrees, according to the Chinese Lunar Exploration Program, after the autumn equinox in late February. Conditions should already by more favorable following the Spring equinox on Dec. 26. Mars has an axial tilt of around 25 degrees, meaning it has has similar seasonal variations to Earth during its orbit around the sun.

While there has so far been no official comment, the rover may have been impacted by sand storms in the area, which could reduce the levels of energy generation. The Tianwen-1 orbiter noted storms around the landing area in March and April 2021.

Zhurong has active means of removing dust from its four butterfly wing solar arrays, but would be unable to perform this operation while hibernating. The arrays also have an anti-dust coating and can tilt to maximize light collection.

Zhurong had a primary mission lifetime of three Earth months but operated for just over one Earth year in Utopia Planitia, traveling at least 1,921 meters south from its landing site. It was seeking out geomorphologic targets such as mud volcanoes during its extended mission.

The rover has returned detailed insights into the local layered subsurface with its ground-penetrating radar and discovered evidence of relatively recent aqueous activity in the area. The rover landing was also used by NASA Administrator Bill Nelson as a warning to Congress as to China’s competitive threat to American leadership in human spaceflight.


Meanwhile the Tianwen-1 orbiter has been tasked with assessing the area and attempting to contact the rover. Teams are however also having trouble receiving data from the orbiter, according to SCMP.

Radio amateurs have also noted issues with attempts for ground stations to lock onto the orbiter.

Tianwen-1 was scheduled to conduct aerobraking tests late last year as part of preparation for a Mars sample return mission potentially launching later this decade. It is unknown if the tests have been conducted and potentially impacted the orbiter. Chinese space authorities have yet to comment on the situation.

The Tianwen-1 orbiter was initially used to assess the pre-selected landing zones for Zhurong. It was then used primarily as a communications relay for Zhurong during the rover’s primary mission phase, before then switching to focus more on its own science objectives.

It completed a mapping of the Martian surface with a medium-resolution camera by June 2022, and also completed its assigned goals for its six science payloads.

Tianwen-1 orbiter

China launched its Tianwen-1 mission to Mars in July 2020 with the combination of the Tianwen-1 orbiter and Zhurong rover entering Mars orbit in February 2021.

Both Tianwen-1 and Zhurong had entered a standby mode in 2021 when the Earth and Mars were orbiting at opposite sides of the sun, causing a communications blackout.

China plans to launch the Tianwen-2 joint near-Earth asteroid sample-return and main belt comet rendezvous mission around 2025.

Related link:

For more information about China National Space Administration (CNSA), visit: http://www.cnsa.gov.cn/

Images, Text, Credits: CNSA/PEC/Twitter/SpaceNews/by Andrew Jones.

Greetings, Orbiter.ch

dimanche 8 janvier 2023

Retired NASA Earth Radiation Budget Satellite to Reenter Atmosphere

 







NASA / GSFC - Earth Radiation Budget Satellite (ERBS) patch.


Jan 8, 2023

In early January NASA’s retired Earth Radiation Budget Satellite (ERBS) is expected to reenter Earth’s atmosphere after almost four decades in space. For 21 of those years, the ERBS actively investigated how the Earth absorbed and radiated energy from the Sun, and made measurements of stratospheric ozone, water vapor, nitrogen dioxide, and aerosols. 

As of Thursday, Jan. 5, the Department of Defense predicted that the 5,400-pound satellite will reenter the atmosphere at approximately 6:40 p.m. EST on Sunday, Jan. 8 with an uncertainty of +/- 17 hours. NASA and the Defense Department will continue to monitor the reentry and update the predictions.

Image above: NASA’s retired Earth Radiation Budget Satellite (ERBS) is expected to reenter Earth’s atmosphere in early January. Image Credit: NASA.

NASA expects most of the satellite to burn up as it travels through the atmosphere, but some components are expected to survive the reentry. The risk of harm coming to anyone on Earth is very low – approximately 1 in 9,400.

Launched from the Space Shuttle Challenger on Oct. 5, 1984, the ERBS spacecraft was part of NASA’s three-satellite Earth Radiation Budget Experiment (ERBE) mission. It carried three instruments, two to measure the Earth's radiative energy budget, and one to measure stratospheric constituents, including ozone. 

The energy budget, the balance between the amount of energy from the Sun that Earth absorbs or radiates, is an important indicator of climate health, and understanding it can also help reveal weather patterns. Ozone concentrations in the stratosphere play an important role in protecting life on Earth from damaging ultraviolet radiation.

Image above: The ERBS was released into orbit by America's first woman in space, Sally Ride. Image Credit: NASA.

ERBS far exceeded its expected two-year service life, operating until its retirement in 2005. Its observations helped researchers measure the effects of human activities on Earth’s radiation balance. NASA has continued to build on the success of the ERBE mission with projects including the current Clouds and the Earth’s Radiant Energy System (CERES) suite of satellite instruments. 

The Stratospheric Aerosol and Gas Experiment II (SAGE II) on the ERBS made stratospheric measurements. SAGE II collected important data that confirmed the ozone layer was declining on a global scale. That data helped shape the international Montreal Protocol Agreement, resulting in a dramatic decrease around the globe in the use of ozone-destroying chlorofluorocarbons. Today, SAGE III on the International Space Station collects data on the health of the ozone layer.

Related link:

Earth Radiation Budget Satellite (ERBS): https://en.wikipedia.org/wiki/Earth_Radiation_Budget_Satellite

Images (mentioned), Text, Credits: NASA/Joe Atkinson.

Greetings, Orbiter.ch