Thursday, September 26, 2024

Views of Hurricane Helene | International Space Station

Views of Hurricane Helene | International Space Station

Cameras on the International Space Station captured views of Hurricane Helene at 2:25 p.m. EDT September 26, 2024, as it approached the Gulf coast of Florida packing winds in excess of 120 miles an hour. The National Hurricane Center forecast called for Helene to continue to strengthen before it makes landfall along the Big Bend region of Florida, then traverses up western Georgia and the Tennessee Valley.

National Hurricane Center Updates:

https://www.nhc.noaa.gov


Expedition 72 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexander Grebenkin, Alexey Ovchinin, Ivan Vagner 
NASA: Matthew Dominick, Mike Barrett, Jeanette Epps, Butch Wilmore, Don Pettit

Video Credit: NASA's Johnson Space Center (JSC)

Duration: 3 minutes, 47 seconds

Release Date: Sept. 26, 2024


#NASA #Space #Science #ISS #Planet #Earth #Atmosphere #Weather #HurricaneHelene #GulfOfMexico #GulfCoast #Astronauts #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition72 #China #中国 #SouthAfrica #STEM #Education #Timelapse #HD #Video    

DECam confirma que los vecindarios de los cuásares del Universo primitivo están realmente abarrotados

DECam confirma que los vecindarios de los cuásares del Universo primitivo están realmente abarrotados

Cosmoview Episodio 86: Observaciones realizadas con la Cámara de Energía Oscura (DECam, por sus siglas en inglés) confirman las expectativas de los astrónomos de que los cuásares del Universo primitivo se formaron en regiones del espacio densamente pobladas con galaxias compañeras. El enorme campo de visión de DECam y sus filtros especiales jugaron un papel fundamental para llegar a esta conclusión. Además, estas observaciones revelan la razón por la que los estudios previos que buscaban caracterizar la densidad de los vecindarios de los cuásares en el Universo primitivo arrojaban resultados contradictorios.


Credit:

Images and Videos: NOIRLab/NSF/AURA/M. Garlick/J. da Silva (Spaceengine)/M. Zamani/CTIO/T. Slovinský/ESO/M. Kornmesser/N. Bartmann

Duration: 1 minute, 17 seconds

Release Date: Sept. 23, 2024


#NASA #Astronomy #Space #Science #español #Quasar #Galaxies #EarlyUniverse #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NSF #AURA #DOE #UnitedStates #STEM #Education #HD #Video

Early-Universe Quasar Neighborhoods Cluttered with Galaxies | NOIRLab

Early-Universe Quasar Neighborhoods Cluttered with Galaxies | NOIRLab

Cosmoview Episode 86: Observations using the Dark Energy Camera (DECam) confirm astronomers’ expectation that early-Universe quasars formed in regions of space densely populated with companion galaxies. DECam’s exceptionally wide field of view and special filters played a crucial role in reaching this conclusion, and the observations reveal why previous studies seeking to characterize the density of early-Universe quasar neighborhoods have yielded conflicting results.

Dark Energy Camera (DECam)

https://www.darkenergysurvey.org/the-des-project/instrument/the-camera/


Credit:

Images and Videos: NOIRLab/NSF/AURA/M. Garlick/J. da Silva/M. Zamani/CTIO/T. Slovinský/ESO/M. Kornmesser/N. Bartmann

Duration: 1 minute, 17 seconds

Release Date: Sept. 23, 2024


#NASA #Astronomy #Space #Science #Quasar #Galaxies #EarlyUniverse #Cosmos #Universe #VictorBlancoTelescope #DECam #CTIO #CerroTololo #Chile #NSF #AURA #DOE #UnitedStates #STEM #Education #HD #Video

Spiral Galaxy NCG 7329 in Tucana | Hubble Space Telescope

Spiral Galaxy NCG 7329 in Tucana | Hubble Space Telescope


This stellar whirlpool is a spiral galaxy named NCG 7329. It was imaged by Hubble’s Wide Field Camera 3 (WFC3). Creating a colorful image using a telescope, such as Hubble, is not as straightforward as pointing and clicking a camera. Commercial cameras will typically try to collect as much light of all visible wavelengths as they can, in order to create the most vibrant images possible. In contrast, raw images collected by Hubble are always monochromatic, because astronomers typically want to capture very specific ranges of wavelengths of light at any time, in order to produce the best, most accurate science possible. In order to control what wavelengths of light will be collected, Hubble’s cameras are equipped with a variety of filters that only allow certain wavelengths of light to reach the cameras’ CCDs. A CCD is a camera light sensor—mobile phone cameras also have CCDs. 

How are colorful Hubble images possible given that raw Hubble images are monochromatic? This is accomplished by combining multiple observations of the same object obtained using a choice of filters. This image, for example, was processed from Hubble observations made using four filters, each of spanning a distinct region of the light spectrum—from the ultraviolet to optical and infrared. Specialized image processors and artists can make informed judgements about the optical colors that best correspond to each filter used. They can then color the images taken using that filter accordingly. Finally, the images taken with each filter are stacked together, and voila! The colorful image of a distant galaxy is complete with colors as representative of reality as possible.


Image Credit: ESA/Hubble & NASA, A. Riess et al.

Release Date: Dec. 6, 2021


#NASA #Hubble #Astronomy #Space #Science #Galaxies #Galaxy #NGC7329 #SpiralGalaxy #Tucana #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education

Black Hole Beams Promote Stellar Eruptions | Hubble Space Telescope

Black Hole Beams Promote Stellar Eruptions | Hubble Space Telescope

Giant galaxy M87 shows a 3,000-light-year-long jet of plasma blasting from the galaxy's 6.5-billion-solar-mass central black hole
Black hole jet and accompanying erupting nova (artist's concept)

In a surprise finding, astronomers using the NASA/European Space Agency Hubble Space Telescope have discovered that the blowtorch-like jet from a supermassive black hole at the core of a huge galaxy seems to cause stars to erupt along its trajectory. The stars, called novae, are not caught inside the jet, but are apparently in a dangerous neighborhood nearby.

The finding confounds researchers searching for an explanation. "We don't know what's going on, but it's just a very exciting finding," said lead author Alec Lessing of Stanford University. "This means there's something missing from our understanding of how black hole jets interact with their surroundings."

A nova erupts in a double-star system where an ageing, swelled-up, normal star spills hydrogen onto a burned-out white dwarf companion star. When the dwarf has tanked up a mile-deep surface layer of hydrogen that layer explodes like a giant nuclear bomb. The white dwarf is not destroyed by the nova eruption. It ejects its surface layer and then goes back to syphoning fuel from its companion, and the nova-outburst cycle starts over again.

Hubble found twice as many novae going off near the jet as elsewhere in the giant galaxy during the surveyed time period. The jet is launched by a 6.5-billion-solar-mass central black hole surrounded by a disc of swirling matter. The black hole, engorged with infalling matter, launches a 3,000-light-year-long jet of plasma blazing through space at nearly the speed of light. Anything caught in the energetic beam would be sizzled. However, being near its blistering outflow is apparently also risky, according to the new Hubble findings.

The finding of twice as many novae near the jet implies that there are twice as many nova-forming double-star systems near the jet or that these systems erupt twice as often as similar systems elsewhere in the galaxy.

"There's something that the jet is doing to the star systems that wander into the surrounding neighborhood. Maybe the jet somehow snowplows hydrogen fuel onto the white dwarfs, causing them to erupt more frequently," said Lessing. "But it's not clear that it's a physical pushing. It could be the effect of the pressure of the light emanating from the jet. When you deliver hydrogen faster, you get eruptions faster. Something might be doubling the mass transfer rate onto the white dwarfs near the jet." Another idea the researchers considered is that the jet is heating the dwarf's companion star, causing it to overflow further and dump more hydrogen onto the dwarf. However, the researchers calculated that this heating is not nearly large enough to have this effect.

"We're not the first people who've said that it looks like there's more activity going on around the M87 jet," said co-investigator Michael Shara of the American Museum of Natural History in New York City. "But Hubble has shown this enhanced activity with far more examples and statistical significance than we ever had before."

Shortly after Hubble's launch in 1990, astronomers used its first-generation Faint Object Camera (FOC) to peer into the center of M87 where the monster black hole lurks 54 million light years away. They noted that unusual things were happening around the black hole. Almost every time Hubble looked, astronomers saw bluish "transient events" that could be evidence for novae popping off like camera flashes from nearby paparazzi. Unfortunately, the FOC's view was so narrow that Hubble astronomers could not look away from the jet to compare with the near-jet region. For over two decades, the results remained mysteriously tantalizing.

Compelling evidence for the jet's influence on the stars of the host galaxy was collected over a nine-month interval when Hubble observed with newer, wider-view cameras to count the erupting novae. This was a challenge for the telescope's observing schedule because it required revisiting M87 precisely every five days for another snapshot. Adding up all of the M87 images led to the deepest images of M87 that have ever been taken. 

Hubble found 94 novae in the one-third of M87 that its camera can encompass. "The jet was not the only thing that we were looking at—we were looking at the entire inner galaxy. Once you plotted all known novae on top of M87 you did not need statistics to convince yourself that there is an excess of novae along the jet. This is not rocket science. We made the discovery simply by looking at the images. And while we were really surprised, our statistical analyses of the data confirmed what we clearly saw," said Shara.

“We are witnessing an intriguing but puzzling phenomenon,” commented Chiara Circosta, a European Space Agency Research Fellow, who studies the impact that accreting supermassive blackholes have on the galaxies hosting them in the distant Universe. “I was very surprised by this discovery. Such detailed observations of nearby galaxies are precious to expand our understanding of how jets interact with their host galaxies and potentially affect star formation”

This accomplishment is entirely due to Hubble's unique capabilities. Ground-based telescope images do not have the clarity to see novae deep inside M87. They cannot resolve stars or stellar eruptions close to the galaxy's core because the black hole's surroundings are far too bright. Only Hubble can detect novae against the bright M87 background. 

Novae are remarkably common in the Universe. One nova erupts somewhere in M87 every day. Moreover, since there are at least 100 billion galaxies throughout the visible universe, around one million novae erupt every second somewhere out there.


Image Credit: NASA, ESA, J. Olmsted (STScI)

Release Date: Sept. 26, 2024


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Novae #Galaxy #M87 #Elliptical Galaxy #BlackHole #BlackHoleJet #VirgoCluster #Virgo #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #Art #Illustration #STEM #Education

Firebird Nebula & NGC 6193 Star Cluster: Infrared view | ESO

Firebird Nebula & NGC 6193 Star Cluster: Infrared view | ESO

This image is filled with densely packed stars, most of them only tiny light blue or orange dots. There are so many stars that the dark sky is almost indiscernible. Towards the center-right there is a dark region with fewer stars and, inside it, a bright orange nebula.

This is an infrared image of NGC 6188, also known as the Firebird Nebula, located about 4,100 light-years away in the constellation Ara. This gas cloud harbors a cluster of young stars called NGC 6193. The image was captured by ESO’s VISTA―the Visible and Infrared Survey Telescope for Astronomy―with its infrared camera VIRCAM. The image is part of a giant infrared map of the Milky Way containing more than 1.5 billion objects. The data for this map were gathered as part of the VISTA Variables in the Vía Láctea (VVV) survey and its companion project, the VVV eXtended survey (VVVX).


Credit: ESO/VVVX survey

Release Date: Sept. 26, 2024


#NASA #ESO #Astronomy #Space #Science #Nebulae #Nebula #NGC6188 #FirebirdNebula #EmissionNebula #StarCluster #NGC6193 #Ara #Constellation #MilkyWayGalaxy #Cosmos #Universe #VISTA #VIRCAM #InfraredTelescope #Chile #Europe #STEM #Education

Messier 17 Nebula: Wide-field infrared view | European Southern Observatory

Messier 17 Nebula: Wide-field infrared view | European Southern Observatory


This image has a small wispy gas cloud at its center. The cloud is orange and pink, its tendrils getting less opaque and more blue to the left. It is surrounded by thousands of tiny dotted blue, orange and yellow stars, very densely packed, giving the background a blue hue. There are darker patches all over the image where fewer stars are showing.

This image shows a detailed infrared view of Messier 17, also known as the Omega Nebula or Swan Nebula, a stellar nursery located about 5,500 light-years away in the constellation Sagittarius. 

This image is part of a record-breaking infrared map of the Milky Way containing more than 1.5 billion objects. The European Southern Observatory’s VISTA―the Visible and Infrared Survey Telescope for Astronomy―captured the images with its infrared camera VIRCAM. The data were gathered as part of the VISTA Variables in the Vía Láctea (VVV) survey and its companion project, the VVV eXtended survey (VVVX).


Credit: ESO/VVVX survey

Release Date: Sept. 26, 2024


#NASA #ESO #Astronomy #Space #Science #Nebula #OmegaNebula #SwanNebula #Messier17 #M17 #StellarNursery #Sagittarius #Constellation #MilkyWayGalaxy #Cosmos #Universe #VISTA #VIRCAM #InfraredTelescope #Chile #Europe #STEM #Education

NASA Analysis Shows Irreversible Sea Level Rise for Pacific Islands | JPL

NASA Analysis Shows Irreversible Sea Level Rise for Pacific Islands | JPL

Overhead view of Pacific island nation Kiribati with 32 atolls in total

Pacific Island nations, such as Kiribati—a low-lying country in the southern Pacific Ocean—are preparing now for a future of higher sea levels. 

Climate change is rapidly reshaping a region of the world that is home to millions of people.

To explore the high-tide flooding maps for Pacific Island nations, go to:

https://sealevel.nasa.gov

In the next 30 years, Pacific Island nations, like Tuvalu, Kiribati, and Fiji will experience at least 8 inches (15 centimeters) of sea level rise, according to an analysis by NASA’s sea level change science team. This amount of rise will occur regardless of whether greenhouse gas emissions change in the coming years.

The sea level change team undertook the analysis of this region at the request of several Pacific Island nations, including Tuvalu and Kiribati, and in close coordination with the U.S. Department of State.

In addition to the overall analysis, the agency’s sea level team produced high-resolution maps showing how Pacific Island nations will be vulnerable to high-tide flooding—otherwise known as nuisance flooding or sunny day flooding—by the 2050s. Released on Sept. 23, 2024, the maps outline flooding potential in a range of emissions scenarios, from best-case to business-as-usual to worst-case.

“Sea level will continue to rise for centuries, causing more frequent flooding,” said Nadya Vinogradova Shiffer, who directs ocean physics programs for NASA’s Earth Science Division. “NASA’s new flood tool tells you what the potential increase in flooding frequency and severity look like in the next decades for the coastal communities of the Pacific Island nations.”

Team members, led by researchers at the University of Hawaii and in collaboration with scientists at the University of Colorado and Virginia Tech, started with flood maps of Kiribati, Tuvalu, Fiji, Nauru, and Niue. They plan to build high-resolution maps for other Pacific Island nations in the near future. The maps can assist Pacific Island nations in deciding where to focus mitigation efforts.

“Science and data can help the community of Tuvalu in relaying accurate sea level rise projections,” said Grace Malie, a youth leader from Tuvalu who is involved with the Rising Nations Initiative, a United Nations-supported program led by Pacific Island nations to help preserve their statehood and protect the rights and heritage of populations affected by climate change. “This will also help with early warning systems, which is something that our country is focusing on at the moment.”

Future Flooding

The analysis by the sea level change team also found that the number of high-tide flooding days in an average year will increase by an order of magnitude for nearly all Pacific Island nations by the 2050s. Portions of the NASA team’s analysis were included in a sea level rise report published by the United Nations in August 2024.

Areas of Tuvalu that currently see less than five high-tide flood days a year could average 25 flood days annually by the 2050s. Regions of Kiribati that see fewer than five flood days a year today will experience an average of 65 flood days annually by the 2050s.

“I am living the reality of climate change,” said Malie. “Everyone (in Tuvalu) lives by the coast or along the coastline, so everyone gets heavily affected by this.”

Flooding on island nations can come from the ocean inundating land during storms or during exceptionally high tides, called king tides. However, it can also result when saltwater intrudes into underground areas and pushes the water table to the surface. “There are points on the island where we will see seawater bubbling from beneath the surface and heavily flooding the area,” Malie added.

Matter of Location

Sea level rise does not occur uniformly around the world. A combination of global and local conditions, such as the topography of a coastline and how glacial meltwater is distributed in the ocean, affects the amount of rise a particular region will experience.

“We’re always focused on the differences in sea level rise from one region to another, but in the Pacific, the numbers are surprisingly consistent,” said Ben Hamlington, a sea level researcher at NASA’s Jet Propulsion Laboratory in Southern California and the agency’s sea level change science team lead.

The impacts of 8 inches (15 centimeters) of sea level rise will vary from country to country. For instance, a number of nations could experience nuisance flooding several times a year at their coastal airports, while others might face frequent neighborhood flooding equivalent to being inundated for nearly half the year.

Researchers would like to combine satellite data on ocean levels with ground-based measurements of sea levels at specific points, as well as with better land elevation information. “But there’s a real lack of on-the-ground data in these countries,” said Hamlington. The combination of space-based and ground-based measurements can yield more precise sea level rise projections and improved understanding of the impacts to countries in the Pacific.

“The future of the young people of Tuvalu is already at stake,” said Malie. “Climate change is more than an environmental crisis. It is about justice, survival for nations like Tuvalu, and global responsibility.”


Credits: NASA's Jet Propulsion Laboratory (JPL)/NASA Earth Observatory

Release Date: Sept. 25, 2024


#NASA #Space #Satellites #Science #Planet #Earth #PacificOcean #SeaLevels #Tuvalu #Kiribati #Fiji #GlobalTemperatureRecords #Weather #Meteorology #ClimateChange #GlobalHeating #Climate #Environment #GreenhouseGases #GHG #EarthObservation #RemoteSensing #JPL #Caltech #GSFC #UnitedStates #STEM #Education

Wednesday, September 25, 2024

NASA's SpaceX Crew-9: Launch Day Practice Session | Kennedy Space Center

NASA's SpaceX Crew-9: Launch Day Practice Session | Kennedy Space Center

NASA’s SpaceX Crew-9 crew members, NASA astronaut Nick Hague (left) and Roscosmos cosmonaut Aleksandr Gorbunov of Russia (right), participate in a countdown dress rehearsal inside the crew suit-up room of the Neil A. Armstrong Operations and Checkout Building at the agency’s Kennedy Space Center in Florida
NASA’s SpaceX Crew-9 crew members: Roscosmos cosmonaut Aleksandr Gorbunov of Russia (left) and NASA astronaut Nick Hague (right)


NASA astronaut Nick Hague, wearing a SpaceX spacesuit, is seen departing the Neil A. Armstrong Operations and Checkout Building for Space Launch Complex 40 at Cape Canaveral

NASA Associate Administrator Jim Free, left, waves farewell as NASA astronaut Nick Hague and Roscosmos cosmonaut Aleksandr Gorbunov of Russia depart the Neil A. Armstrong Operations and Checkout Building for Space Launch Complex 40
The official portrait of the International Space Station's Expedition 72 crew. At the top (from left) are, Roscosmos cosmonaut and Flight Engineer Alexey Ovchinin (Russia), NASA astronaut and space station Commander Suni Williams, and NASA astronaut and Flight Engineer Butch Wilmore. In the middle row are, Roscosmos cosmonaut and Flight Engineer Ivan Vagner (Russia) and NASA astronaut and Flight Engineer Don Pettit. In the bottom row are, Roscosmos cosmonaut and Flight Engineer Aleksandr Gorbunov (Russia) and NASA astronaut and Flight Engineer Nick Hague.

NASA astronaut Nick Hague and Roscosmos cosmonaut Aleksandr Gorbunov of Russia, wearing SpaceX spacesuits, are seen as they depart the Neil A. Armstrong Operations and Checkout Building for Space Launch Complex 40 at Cape Canaveral during a dress rehearsal in preparation for the Crew-9 mission launch, Tuesday, Sept. 24, 2024, at NASA’s Kennedy Space Center in Florida. Launch is targeted for no earlier than 1:17 p.m. EDT Saturday, Sept. 28, 2024. 

For more on Crew-9, visit: 

This is the ninth rotational mission to the space station under NASA’s Commercial Crew Program. It works with the American aerospace industry to meet the goal of safe, reliable, and cost-effective transportation to and from the orbital outpost on American-made rockets and spacecraft launching from American soil.

More information on NASA’s Commercial Crew Program:

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexander Grebenkin, Alexey Ovchinin, Ivan Vagner 
NASA: Matthew Dominick, Mike Barrett, Jeanette Epps, Butch Wilmore, Don Pettit

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.

Image Credits: NASA/Keegan Barber/Kim Shiflett/Bill Stafford/Robert Markowitz
Capture Date: Sept. 24, 2024

#NASA #Space #ISS #Science #SpaceXCrew9 #SpaceX #CrewDragonSpacecraft #Falcon9Rocket #Astronaut #NickHague #Cosmonaut #AleksandrGorbunov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #CCP #Expedition72 #KSC #CapeCanaveral #Florida #UnitedStates #STEM #Education

NASA "Espacio a Tierra" | El camino por delante: 06 de septiembre de 2024

NASA "Espacio a Tierra" | El camino por delante: 06 de septiembre de 2024

Espacio a Tierra, la versión en español de las cápsulas Space to Ground de la NASA, te informa semanalmente de lo que está sucediendo en la Estación Espacial Internacional.

Aprende más sobre la ciencia a bordo de la estación espacial:

https://www.nasa.gov/international-space-station/space-station-research-and-technology/ciencia-en-la-estacion/

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: 

https://www.nasa.gov/suscribete

Ciencia de la NASA: https://ciencia.nasa.gov


Video Credit: NASA's Johnson Space Center (JSC)

Duration: 3 minutes, 34 seconds

Release Date: Sept. 25, 2024


#NASA #Space #ISS #Science #NASAenespañol #español #SpaceXCrew9 #Astronauts #NickHague #SunitaWilliams #UnitedStates #Cosmonauts #AleksandrGorbunov #Russia #Россия #Roscosmos #Роскосмос #SpaceLaboratory #Expedition71 #Expedition72 #HumanSpaceflight #InternationalCooperation #STEM #Education #HD #Video

Russian Soyuz MS-25 Crew Spacecraft Departs International Space Station

Russian Soyuz MS-25 Crew Spacecraft Departs International Space Station





Soyuz MS-25 crew members (from left to right): NASA astronaut Tracy C. Dyson and Roscosmos cosmonauts Oleg Kononenko and Nikolai Chub of Russia
 
The Russian Soyuz MS-25 spacecraft, with NASA astronaut Tracy C. Dyson and Roscosmos cosmonauts Nikolai Chub and Oleg Kononenko of Russia aboard, is pictured shortly after undocking from the International Space Station's Prichal module.

On Sept. 23, 2024, the Soyuz MS-25 spacecraft made a parachute-assisted landing on the steppe of Kazakhstan, southeast of the town of Dzhezkazgan.

Spanning 184 days in space, NASA astronaut Tracy C. Dyson’s mission includes covering 2,944 orbits of the Earth and a journey of 78 million miles. The Soyuz MS-25 spacecraft launched March 23, 2024, and arrived at the International Space Station March 25, with Dyson, Roscosmos cosmonaut Oleg Novitskiy of Russia, and cosmonaut Marina Vasilevskaya of Belarus.

Roscosmos cosmonauts Nikolai Chub and Oleg Kononenko, who launched with O’Hara to the station on the Soyuz MS-24 spacecraft last September, returned after 374 days in space and a trip of 158.6 million miles, spanning 5,984 orbits.

Dyson spent her third spaceflight aboard the station as an Expedition 70 and 71 flight engineer, and returned with Kononenko, completing his fifth flight into space and accruing an all-time record of 1,111 days in orbit, along with Chub, who completed his first spaceflight.

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.

Expedition 72 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 72 Crew

Station Commander: Suni Williams

Roscosmos (Russia): Alexander Grebenkin, Alexey Ovchinin, Ivan Vagner 

NASA: Matthew Dominick, Mike Barrett, Jeanette Epps, Butch Wilmore, Don Pettit


Image Credit: NASA's Johnson Space Center (JSC)

Capture Date: Sept. 23, 2024


#NASA #Space #ISS #Science #Earth #SoyuzSpacecraft #SoyuzMS25 #Astronaut #TracyDyson #UnitedStates #Cosmonauts #OlegKononenko #NikolaiChub #Russia #Россия #Roscosmos #Роскосмос #SpaceLaboratory #Expedition71 #Expedition72 #HumanSpaceflight #InternationalCooperation #STEM #Education

Comet Tsuchinshan-ATLAS (C/2023 A3) | International Space Station

Comet Tsuchinshan-ATLAS (C/2023 A3) | International Space Station

NASA Astronaut Matthew Dominick: "The comet tail is noticeably longer each day. Pause the video at about 15 seconds . . . you can see the tail of the comet looks like it is bending. The atmosphere is more dense the closer you get to earth. Changes in the density of the atmosphere change the refractive index and thus make the comet tail appear bent."

"I was in my crew quarters reviewing the imagery when I first saw the bend in the comet’s tail. I did not see it real time when taking the images. I yelled out the door to to check it out but he was already off to take more images of the comet with an IR camera . . . look forward to those."

"Video is a timelapse played at 8 frames per second. Images were taken with a 1/8 sec exposure with about 5ms in between shots so this timelapse should be about the same speed as we see it out the window."

"Canadarm2 is in the near field, upper left, and out of focus." 

Technical details: 200mm, 1/8s, ISO 5000

C/2023 A3 (Tsuchinshan–ATLAS) is a comet from the solar system's Oort cloud discovered by the Purple Mountain Observatory east of Nanjing, China, on January 9, 2023, and independently found by the automated Asteroid Terrestrial-impact Last Alert System (ATLAS) in South Africa on February 22, 2023. ATLAS is funded by NASA's planetary defense office, and developed and operated by the University of Hawaii's Institute for Astronomy. C/2023 A3 will pass perihelion (closest approach to the Sun) at a distance of 0.39 AU (58 million km; 36 million miles) on September 27, 2024. This is when it can be best viewed with the naked eye from the ground on Earth.

The Oort cloud is theorized to be a vast cloud of icy planetesimals surrounding the Sun at distances ranging from 2,000 to 200,000 AU (0.03 to 3.2 light-years). The concept of such a cloud was proposed in 1950 by the Dutch astronomer Jan Oort, in whose honor the idea was named. Oort proposed that the bodies in this cloud replenish and keep constant the number of long-period comets entering the inner Solar System—where they are eventually consumed and destroyed during close approaches to the Sun.

Expedition 72 Updates:

https://blogs.nasa.gov/spacestation/

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexander Grebenkin, Alexey Ovchinin, Ivan Vagner 
NASA: Matthew Dominick, Mike Barrett, Jeanette Epps, Butch Wilmore, Don Pettit

Video Credit: NASA's Johnson Space Center/M. Dominick

Duration: 1 minute

Release Date: Sept. 25, 2024


#NASA #Space #Science #ISS #Planet #Earth #Comets #CometTsuchinshanATLAS #C2023A3 #OortCloud #SolarSystem #Astronaut #MatthewDominick #AstronautPhotography #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition72 #China #中国 #SouthAfrica #STEM #Education #Timelapse #HD #Video

To an Asteroid and Back: Full-length Documentary Released | NASA Goddard

To an Asteroid and Back: Full-length Documentary Released | NASA Goddard

 

In a full-length documentary film, follow along with NASA's OSIRIS-REx team as they launch a spacecraft to an asteroid, collect a sample of Bennu, and bring it home to Earth. 

Watch the new documentary here: https://plus.nasa.gov/video/to-an-asteroid-and-back/

OSIRIS-REx NASA page: https://www.nasa.gov/osiris-rex

University of Arizona's OSIRIS-REx Mission Page: http://www.asteroidmission.org

Follow sample-delivery updates on NASA's OSIRIS-REx blog: 

https://blogs.nasa.gov/osiris-rex/


Credit: NASA's Goddard Space Flight Center

Producer: James Tralie

Duration: 1 minute, 27 seconds

Release Date: Sept. 24, 2024

#NASA #Astronomy #Space #Science #OSIRISRExMission #OSIRISRExSpacecraft #Asteroids #AstreroidBennu #ToBennuAndBack #SampleReturn #SpaceTechnology #CSA #Canada #CNES #France #JSC #GSFC #UArizona #JSC #UnitedStates #SolarSystem #SpaceExploration #STEM #Education #Documentary #HD #Video

Possible Clays near Margaritifer Chaos | NASA's Mars Reconnaissance Orbiter

Possible Clays near Margaritifer Chaos | NASA's Mars Reconnaissance Orbiter

The term chaos is applied to regions where the surface is being eroded to form mesas separated by steep walled valleys. As the surface processes continue individual mesas become more isolated and take on the appearance of regions of hills. 

The Margaritifer Sinus quadrangle covers the area from 0° to 45° west longitude and 0° to 30° south latitude on Mars. According to the Mars Reconnaissance Orbiter's Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) multispectral data, the exposures of light-toned materials (on small hills and between darker dunes) shows a strong iron-magnesium phyllosilicate (clay) signatures in this area. Phyllosilicates, or sheet silicates, are an important group of minerals that includes the micas, chlorite, serpentine, talc, and the clay minerals. The existence of clay minerals is especially interesting on Mars since we want to know under what conditions these minerals formed. Could it have been in the presence of water?

Image cutout is less than 1 km (under 1 mi) across and the spacecraft altitude was 263 km (164 mi). 

The High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter captured this image.

Mars Reconnaissance Orbiter (MRO) is a spacecraft designed to study the geology and climate of Mars, to provide reconnaissance of future landing sites, and to relay data from surface missions back to Earth. It was launched on August 12, 2005, and reached Mars on March 10, 2006. 

The Jet Propulsion Laboratory (JPL) manages MRO for NASA’s Science Mission Directorate in Washington. Caltech, in Pasadena, manages JPL for NASA. The University of Arizona, in Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., in Boulder, Colorado. The Context Camera was built by, and is operated by, Malin Space Science Systems in San Diego.

For more information on MRO, visit:

https://mars.nasa.gov/mro

https://www.nasa.gov/mission_pages/MRO/mission/index.html


Image Credit: NASA/JPL-Caltech/University of Arizona

Release Date: Sept. 24, 2024


#NASA #Space #Astronomy #Mars #Planet #RedPlanet #Science #Geology #Landscape #Terrain #MargaritiferChaos #Clays #Geoscience #MRO #Orbiter #Spacecraft #HiRISECamera #JPL #Caltech #BallAerospace #MSSS #STEM #Education

Tuesday, September 24, 2024

Arctic Sea Ice Near Historic Low & Antarctic Ice Continues Decline | NASA Earth

Arctic Sea Ice Near Historic Low & Antarctic Ice Continues Decline | NASA Earth

This summer, Arctic sea ice decreased to a its minimum extent on September 11, 2024. According to the National Snow and Ice Data Center this is the 7th lowest in the satellite record). The decline continues the long-term trend of shrinking ice cover in the Arctic Ocean. Each year, Arctic sea ice melts and refreezes with seasonal changes. 

For 46 years, satellites have been monitoring changes in Arctic sea ice. This long-term data has helped scientists understand how polar environments respond to rising temperatures and extended melting seasons. Meanwhile, Antarctic sea ice is approaching its maximum extent for the year, with time still remaining in the growth season.

Learn more at NASA Climate Change:

https://climate.nasa.gov


Credit: NASA's Goddard Space Flight Center

Grace Weikert (NASA/AMA): Lead Producer

Sally Younger (NASA JPL): Lead Writer

Walt Meier (NASA GSFC): Lead Scientist

Trent L. Schindler (NASA/USRA): Lead Visualizer

Kathleen Gaeta (NASA/AIMMS): Producer 

Duration: 2 minutes

Release Date: Sept. 24, 2024


#NASA #Space #Satellites #Science #Planet #Earth #Arctic #ArcticOcean #Antarctica #SouthernOcean #SeaIce #MeltingIce #Environment #ClimateChange #GlobalWarming #GlobalHeating #Atmosphere #EarthObservation #RemoteSensing #GSFC #UnitedStates #STEM #Education #HD #Video

NASA's SpaceX Crew-9 Preparing for Launch | International Space Station

NASA's SpaceX Crew-9 Preparing for Launch | International Space Station

NASA's SpaceX Crew-9 members astronaut Nick Hague and cosmonaut Aleksandr Gorbunov of Russia
NASA's SpaceX Crew-9 members cosmonaut Aleksandr Gorbunov of Russia and NASA astronaut Nick Hague
SpaceX Crew-9 pilot & commander Nick Hague
SpaceX Crew-9 mission specialist Aleksandr Gorbunov of Russia
NASA's SpaceX Crew-9 crew members Nick Hague and cosmonaut Aleksandr Gorbunov of Russia smile for a photo ahead of their launch
NASA's SpaceX Crew-9 crew members Nick Hague and cosmonaut Aleksandr Gorbunov are pictured completing their training before their mission to the International Space Station
NASA's SpaceX Crew-9 crew members Nick Hague and cosmonaut Aleksandr Gorbunov focus on final preparations for launch aboard Dragon during training at SpaceX headquarters in Hawthorne, California
NASA astronaut Nick Hague (left) and Roscosmos cosmonaut Aleksandr Gorbunov of Russia pose inside the Astronaut Crew Quarters in the Neil A. Armstrong Operations and Checkout Building at NASA’s Kennedy Space Center in Florida

NASA's SpaceX Crew-9 crew members Nick Hague and cosmonaut Aleksandr Gorbunov of Russia are preparing for launch to the International Space Station where they will join Expedition 72. This trip will mark Hague's second visit to the orbiting laboratory and Gorbunov's first. NASA and SpaceX teams have adjusted the next launch opportunity for the Crew-9 Mission to no earlier than 1:17pm ET, Saturday, Sept. 28, 2024, from Space Launch Complex 40 in Cape Canaveral. This is due to tropical storm conditions in the area.

Gorbunov was born in Zheleznogorsk, Kursk region, Russia. He studied engineering with qualifications in spacecraft and upper stages from the Moscow Aviation Institute. Gorbunov graduated from the military department with a specialty in operation and repair of aircraft, helicopters, and aircraft engines. Before being selected as a cosmonaut in 2018, he worked as an engineer for Rocket Space Corporation Energia and supported cargo spacecraft launches from the Baikonur cosmodrome.


Note: Two original SpaceX Crew-9 Mission members, specialist Stephanie Wilson and commander Zena Cardman will have their flights rescheduled due to the need for Suni Williams and Butch Wilmore to remain aborad the space station much longer than planned.

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.

This is the ninth rotational mission to the space station under NASA’s Commercial Crew Program. It works with the American aerospace industry to meet the goal of safe, reliable, and cost-effective transportation to and from the orbital outpost on American-made rockets and spacecraft launching from American soil.

More information on NASA’s Commercial Crew Program:

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexander Grebenkin, Alexey Ovchinin, Ivan Vagner 
NASA: Matthew Dominick, Mike Barrett, Jeanette Epps, Butch Wilmore, Don Pettit

Image Credit: NASA/Kim Shiflett/SpaceX
Image Dates: Jan. 14, 2024 - Sept. 23, 2024

#NASA #Space #ISS #Science #SpaceXCrew9 #SpaceX #CrewDragonSpacecraft #Falcon9Rocket #Astronaut #NickHague #JSC #Cosmonaut #AleksandrGorbunov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #CCP #Expedition72 #California #Florida #UnitedStates #STEM #Education