Thursday, September 26, 2024

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

Comet C/2023 A3 (Tsuchinshan-ATLAS) over Chile

Comet C/2023 A3 (Tsuchinshan-ATLAS) over Chile

Astrophotographer Yuri Beletsky: "I captured this image this morning at 09:22 UTC from Carnegie Las Campanas observatory in the Atacama desert in Chile. The view was absolutely spectacular! The clouds were constantly moving just above the horizon, but we got really lucky when the comet suddenly appeared just above the layer of clouds. I used a Nikon D810a camera + 135mm lens. This is a stack of 15 x 5 sec exposures."

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.

Las Campanas Observatory

Image Credit: Yuri Beletsky

Yuri's website: 

https://www.instagram.com/yuribeletsky/

Location: Las Campanas Observatory, Chile

Image Date: Sept. 24, 2024


#NASA #Space #Astronomy #Science #Planet #Earth #Comets #CometTsuchinshanATLAS #C2023A3 #OortCloud #SolarSystem #Astrophotography #Astrophotographer #YuriBeletsky #LasCampanasObservatory #AtacamaDesert #Chile #SouthAmerica #China #中国 #SouthAfrica
#STEM #Education

China's Smart Dragon-3 Rocket Successfully Launches 8 Satellites by Sea

China's Smart Dragon-3 Rocket Successfully Launches 8 Satellites by Sea

 China successfully launched a Smart Dragon-3 (Jielong-3) 4-stage solid-fueled carrier rocket from the waters near the city of Haiyang in east China's Shandong Province at 10:31am Beijing time on Tuesday, Sept. 24, 2024, placing eight satellites into their designated orbits. The commercial rocket carried satellites, including Tianyi-41, Xing Shi Dai-15/21/22, YuXing-2-05, Fudan-1, Tianyan-15, and Jitianxing A-01.

This launch marks the 4th flight mission for the Smart Dragon-3 carrier rocket series. The Smart Dragon-3 rocket was developed by the China Academy of Launch Vehicle Technology (CALT).

The Taiyuan Satellite Launch Center, headquartered inland in north China's Shanxi province, carried out this offshore launch.


Video Credit: CCTV

Duration: 19 seconds

Release Date: Sept. 24, 2024


#NASA #Space #Satellites #Earth #China #中国 #SmartDragon3Rocket #Jielong3Rocket #捷龙三号运载火箭 #SD3Rocket #SolidFueledRocket #SeaLaunch #RocketLaunch #CALT #CASC #Spaceflight #SpaceTechnology #CommercialSpace #TSLC #Haiyang #Shandong #STEM #Education #HD #Video

The Veil Nebula | Hubble’s Inside the Image | NASA Goddard

The Veil Nebula Hubble’s Inside the Image | NASA Goddard

NASA's Hubble Space Telescope has captured a breathtaking image of the Veil Nebula, a remnant of a supernova explosion that showcases delicate, wispy filaments of ionized gas.

In this video, Dr. Ken Carpenter delves into the stunning details of the Veil Nebula and explains how Hubble's observations shed light on the complex processes involved in the aftermath of a star's explosive death. 

The Veil Nebula lies around 2,100 light-years from Earth in the constellation of Cygnus (The Swan), making it a relatively close neighbor in astronomical terms.

The Veil Nebula is the visible portion of the nearby Cygnus Loop, a supernova remnant formed roughly 10,000 years ago by the death of a massive star. The Veil Nebula’s progenitor star—20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy. Despite this stellar violence, the shockwaves and debris from the supernova sculpted the Veil Nebula’s delicate tracery of ionized gas—creating a scene of surprising astronomical beauty.


Credit: NASA's Goddard Space Flight Center 

Producer, Director & Editor: James Leigh

Director of Photography: James Ball

Executive Producers: James Leigh & Matthew Duncan

Production & Post: Origin Films 

Duration: 3 minutes, 26 seconds

Release Date: Sept. 24, 2024


#NASA #ESA #Astronomy #Space #Science #Hubble #Nebula #VeilNebula #SupernovaRemnant #Cygnus #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #WFC3 #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Ten Years at Mars with NASA’s MAVEN Mission | NASA Goddard

Ten Years at Mars with NASA’s MAVEN Mission | NASA Goddard


On September 21, 2014, NASA’s Mars Atmospheric and Volatile Evolution (MAVEN) spacecraft entered orbit around Mars, beginning its ongoing exploration of the Red Planet’s upper atmosphere. The mission has produced a wealth of data about how Mars’     atmosphere responds to the Sun and solar wind, and how these interactions can explain the loss of the Martian atmosphere to space. Now, as MAVEN continues its mission, we can look back on the remarkable discoveries of its first ten years at Mars.


In celebration of this mission milestone, we recap examples of the most significant scientific results of this unique and long-lasting Mars aeronomy mission:


Extreme atmospheric erosion

One of MAVEN’s first big results was discovering that the erosion of Mars’ atmosphere increases significantly during solar storms. The team studied how the solar wind—a stream of charged particles continually streaming from the Sun—and solar storms continually strip away Mars’ atmosphere, and how this process played a key role in altering the Martian climate from a potentially habitable planet to today’s cold, arid planet.


Sputtering to space 

To better understand how Mars lost much of its atmosphere, MAVEN measured isotopes of argon gas in the upper Martian atmosphere. Argon is a noble gas, meaning it rarely reacts with other constituents in the Martian atmosphere. The only way it can be removed is by atmospheric sputtering—a process where ions crash into the Martian atmosphere at high enough speeds that they knock gas molecules out of the atmosphere. When the MAVEN team analyzed argon isotopes in the upper atmosphere, they were able to estimate that roughly 65% of the argon originally present had been lost through sputtering over the planet’s history.


A new type of aurora

MAVEN has discovered several types of auroras that flare up when energetic particles plunge into the atmosphere, bombarding gases and making them glow. The MAVEN team showed that protons, rather than electrons, create auroras at Mars. On Earth, proton auroras only occur in very small regions near the poles, whereas at Mars they can happen everywhere.


Martian dust storm

In 2018, a runaway series of dust storms created a dust cloud so large that it enveloped the planet. The MAVEN team studied how this “global” dust storm affected Mars’ upper atmosphere to understand how these events affect how the escape of water to space. It confirmed that heating from dust storms can loft water molecules far higher into the atmosphere than usual, leading to a sudden surge in water lost to space.


Map of Martian winds

MAVEN researchers created the first map of wind circulation in the upper atmosphere of Mars. The new map is helping scientists better understand the Martian climate, including how terrain on the planet’s surface is disturbing high-altitude wind currents. The results provide insight into how the dynamics of the upper Martian atmosphere have influenced the Red Planet’s climate evolution in the past and present.


Twisted tail

Mars has an invisible magnetic “tail” that is twisted by its interaction with the solar wind. Although models predicted that magnetic reconnection causes Mars’ magnetotail to twist, it wasn’t until MAVEN arrived that scientists could confirm that the predictions were correct. The process that creates the twisted tail could also allow some of Mars’ already thin atmosphere to escape to space.


Mapping electric currents

Researchers used MAVEN data to create a map of electric current systems in the Martian atmosphere. These form when solar wind ions and electrons smash into the planet’s induced magnetic field, causing the particles to flow apart. The resulting electric currents, which drape around the planet, play a fundamental role in the atmospheric loss that transformed Mars from a world that could have supported life to an inhospitable desert.


Disappearing solar wind

MAVEN recently observed the unexpected “disappearance” of the solar wind. This was caused by a type of solar event so powerful that it created a void in its wake as it traveled across the solar system. MAVEN’s measurements showed that when it reached Mars, the solar wind density dropped significantly. This disappearance of the solar wind allowed the Martian atmosphere and magnetosphere to balloon out by thousands of kilometers.


Ultraviolet views of the Red Planet

MAVEN captured stunning views of Mars in two ultraviolet images taken at different points along the Red Planet’s orbit around the Sun. By viewing the planet in ultraviolet wavelengths, scientists gain insight into the Martian atmosphere and view surface features in remarkable ways.


MAVEN’s principal investigator is based at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado Boulder. LASP is also responsible for managing science operations and public outreach and communications. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space built the spacecraft and is responsible for mission operations. NASA’s Jet Propulsion Laboratory in Southern California provides navigation and Deep Space Network support.

Learn more about MAVEN:

https://lasp.colorado.edu/maven/

https://science.nasa.gov/mission/maven/


Video Credit: NASA's Goddard Space Flight Center

Duration: 6 minutes

Release Date: Sept. 23, 2024

#NASA #Space #Astronomy #Science #Star #Sun #SolarMax #Planet #Mars #Atmosphere #Ultraviolet #UV #Radiation #MAVENMission #MAVENSpacecraft #SolarSystem #SpaceExploration #GSFC #LASP #CUBoulder #UnitedStates #STEM #Education #HD #Video

Monday, September 23, 2024

BBC Star Diary: Catch Sight of Saturn’s Moon Titan | September 23-29, 2024

BBC Star Diary: Catch Sight of Saturn’s Moon Titan September 23-29, 2024

The ringed planet’s moon will be visible just above the northern pole, and a telescope should be able to pick out six other moons. Find out how you can see them for yourself, as well as all the latest stargazing highlights, in this week’s Star Diary podcast, from the makers of BBC Sky at Night Magazine. 

Observe Saturn’s moons: https://www.skyatnightmagazine.com/advice/skills/how-observe-saturn-moons


Video Credit: BBC Sky at Night Magazine

Duration: 12 minutes

Release Date: Sept. 22, 2024


#NASA #Space #Astronomy #Science #Earth #Supermoon #Moon #Planets #Saturn #Titan #SolarSystem #Stars #Constellations #StarClusters #MilkyWayGalaxy #Universe #Skywatching #BBC #UK #Britain #Europe #UnitedStates #Canada #NorthernHemisphere #STEM #Education #Podcast #HD #Video

Pan of Spiral Galaxy IC 1954 in Horologium | Hubble Space Telescope

Pan of Spiral Galaxy IC 1954 in Horologium | Hubble Space Telescope


The spiral galaxy IC 1954, located 45 million light-years from Earth in the constellation Horologium, is the star of this new picture from the Hubble Space Telescope. It sports a glowing bar in its core, two main majestically winding spiral arms and clouds of dark dust across it. An image of this galaxy was previously released in 2021. This image now includes H-alpha data. The improved coverage of star-forming nebulae, prominent emitters of the red H-alpha light, can be seen in the numerous glowing, pink spots across the disc of the galaxy. Interestingly, astronomers posit that the galaxy’s ‘bar’ is actually an energetic star-forming region that just happens to lie over the galactic center.

The new data featured in this image come from a program to extend the cooperation between observatories: Hubble, the infrared James Webb Space Telescope, and the Atacama Large Millimeter/submillimeter Array, a ground-based radio telescope. By surveying IC 1954 and over fifty other nearby galaxies in radio, infrared, optical, and ultraviolet light, astronomers aim to fully trace and reconstruct the path matter takes through stars and the interstellar gas and dust in each galaxy. Hubble’s observing capabilities form an important part of this survey: it can capture younger stars and star clusters when they are brightest at ultraviolet and optical wavelengths, and its H-alpha filter effectively tracks emission from nebulae. The resulting dataset will a valuable resource for research on the evolution of stars in galaxies. 

Image Description: A spiral galaxy seen tilted diagonally. It has two large, curling arms that extend from the center and wrap around. The arms are followed by thick strands of dark reddish dust. The arms and rest of the galaxy’s disc are speckled with glowing patches; a number are blue in color, others are pink, showing gas illuminated by new stars. A faint glow surrounds the galaxy. It lies on a dark, nearly empty background.


Credit: European Space Agency/Hubble & NASA, D. Thilker, J. Lee and the PHANGS-HST Team, N. Bartmann (ESA/Hubble)

Duration: 30 seconds

Release Date: Sept. 23, 2024


#NASA #Hubble #Astronomy #Space #Science #Galaxies #IC1954 #Horologium #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video