Friday, November 08, 2024

NASA's Space to Ground: Location, Location, Location | Week of Nov. 8, 2024

NASA's Space to Ground: Location, Location, Location | Week of Nov. 8, 2024

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. The SpaceX Dragon Freedom spacecraft, with Expedition 72 crew members NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore, as well as Roscosmos cosmonaut Aleksandr Gorbunov, autonomously redocked with the space-facing port of the station’s Harmony module on November 3, 2024.

The port relocation freed up Harmony’s forward-facing port for the 31st SpaceX commercial resupply services mission to the International Space Station. This was the fifth port relocation of a Dragon spacecraft with crew aboard following previous moves during the Crew-1, Crew-2, Crew-6, and Crew-8 missions.

Expedition 72 Updates:

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

Expedition 72 Crew

Station Commander: Suni Williams

Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov

NASA: Butch Wilmore, Don Pettit, Nick Hague

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.

Learn more about the important research being operated on Station:

https://www.nasa.gov/iss-science 

For more information about STEM on Station:

https://www.nasa.gov/stemonstation

Science, Technology, Engineering, Math (STEM)


Video Credit: NASA's Johnson Space Center (JSC)
Duration: 3 minutes, 10 seconds 
Release Date: Nov. 8, 2024


#NASA #Space #Science #ISS #Earth #SpaceX #CRS31 #CargoDragonSpacecraft #SpaceXCrew9 #CrewDragonSpacecraft #CrewDragonFreedom #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education #HD #Video

Thursday, November 07, 2024

Hurricane Rafael after Crossing Cuba | NOAA GOES 16 Weather Satellite

Hurricane Rafael after Crossing Cuba | NOAA GOES 16 Weather Satellite



The latest major storm in 2024’s active hurricane season brought heavy rain and storm surge to Cuba as it moved into the Gulf of Mexico. Hurricane Rafael made landfall in the western Cuban province of Artemisa as a Category 3 storm on the afternoon of November 6, 2024. The hurricane approached the island from the south, having skirted past Jamaica the previous day as a tropical storm. Approaching Cuba, it traversed warm waters and encountered light to moderate vertical wind shear—environmental conditions that helped the storm to strengthen into a major hurricane.

Rafael’s sustained wind speeds peaked at 115 miles (185 kilometers) per hour prior to landfall, reported the National Hurricane Center (NHC). It weakened slightly upon encountering land, downgrading to a Category 2 storm as it moved across Cuba and tracked northwest into the Gulf of Mexico.

According to news reports, the Cuban government announced the hurricane had knocked out power across the entire island before landfall. Several airports suspended flights. Western Cuba was expected to receive 4 to 8 inches (100 to 200 millimeters) of rainfall from the storm system, according to the NHC, with several inches also forecast for the Cayman Islands and Florida Keys. The NHC also warned of strong storm surge that could raise water as much as 14 feet (about 4 meters) above normal levels along Cuba’s southern coast.

As of the morning of November 7, forecasters expected Rafael to move slowly to the west and remain a hurricane for several days, though it could weaken as it encounters a dry airmass in the southern Gulf of Mexico. The longer-term forecast remained uncertain.

Consistent with National Weather Service predictions, it has been an active year for hurricanes in the North Atlantic. Rafael is the 17th named storm and 11th hurricane of the 2024 season, which runs from June 1 to November 30. These numbers exceed the average seasonal totals of 14 named storms and seven hurricanes.

GOES-16 is the first of the GOES-R series of Geostationary Operational Environmental Satellites (GOES) operated by NASA and the National Oceanic and Atmospheric Administration (NOAA). GOES-16 serves as the operational geostationary weather satellite in the GOES East position at 75.2°W, providing a view centered on the Americas. GOES-16 provides high spatial and temporal resolution imagery of the Earth through 16 spectral bands at visible and infrared wavelengths using its Advanced Baseline Imager (ABI). GOES-16 was launched from Cape Canaveral in November 2016 aboard a United Launch Alliance (ULA) Atlas V rocket.


Image Credit: National Oceanic and Atmospheric Administration (NOAA)
NASA Article Credit: Lindsey Doermann
Release Date: Nov. 7, 2024


#NASA #NOAA #Space #Satellites #GOES16 #GOESEast #Science #Planet #Earth #Atmosphere #Meteorology #Weather #Oceans #AtlanticOcean #GulfOfMexico #Cuba #HurricaneRafael #SeaTemperatures #ClimateChange #GlobalHeating #Environment #CIRA #UnitedStates #STEM #Education #Timelapse #Animation #GIF

Ancient Impact Crater & 'Eye' of Quebec in Canada | Landsat 8 Satellite | USGS

Ancient Impact Crater & 'Eye' of Quebec in Canada | Landsat 8 Satellite | USGS

A large, round lake in Quebec, Canada, highlights the geography of an ancient impact crater. In the late Triassic Period, a 3 mile wide meteorite struck northern Pangea at over 30,000 miles per hour. The resulting crater is now 214 million years old, but the dramatic circular lake visible in 2024 Landsat imagery is a surprisingly recent feature.

It was the completion of the Daniel-Johnson Dam in 1968 that united two river systems, creating the Manicouagan Reservoir, or the Eye of Quebec. A declassified 1964 satellite image from the CIA’s Project Argon shows two crescent-shaped lakes originally outlining the impact zone. By 1972, the reservoir’s new water level had been established, as revealed by Landsat 1, with more or less the same shoreline it has today.

The Landsat program conceived of in the 1960s, has been running longer than any remote sensing program. The idea was simple: position a satellite in a nearly polar orbit fixed to the solar angle so that each daytime pass would cross the equator at roughly the same local time.

Data representing bands of the spectrum are captured and processed into grayscale recordings that can be combined to create natural looking views like this or false color views like this. Nine Landsat satellites have been launched in partnership with NASA since 1972.

The USGS EROS Center archive contains a wealth of satellite and digitized film imagery available at no cost to communities and scientists studying land change around the world: 

https://www.usgs.gov/centers/eros/science/usgs-eros-archive-products-overview

Official Quebec Tourism Website:

https://www.bonjourquebec.com/en

Côte-Nord: 

https://www.bonjourquebec.com/en/where-to-go/regions-of-quebec/cote-nord

Station Uapishka S.E.N.C.: 

https://www.bonjourquebec.com/en/listing/accommodation/station-uapishka-s-e-n-c/0a5a


Video Credit: United States Geological Survey (USGS)
Duration: 1 minute, 22 seconds
Release Date: Nov. 7, 2024

#NASA #USGS #Space #Planet #Earth #Geology #Meteorite #Pangea #ImpactCrater #Crater #ManicouaganReservoir #EyeOfQuebec #Quebec #Canada #Satellites #Landsat #Landsat8 #RemoteSensing #EarthObservation #EROS #SouthDakota #GSFC #UnitedStates #International #History #STEM #Education #HD #Video

Close-up: The 'Phantoms' of Star Gamma Cassiopeia—Nebulae IC 59 & IC 63

Close-up: The 'Phantoms' of Star Gamma Cassiopeia—Nebulae IC 59 & IC 63

These brightly outlined flowing shapes look ghostly on a cosmic scale. A telescopic view toward the constellation Cassiopeia, the colorful skyscape features the swept-back, comet-shaped clouds IC 59 (left) and IC 63. About 600 light-years distant, the clouds are not actually ghosts. They are slowly disappearing though, under the influence of energetic radiation from hot, luminous star gamma Cas. 

Gamma Cas is physically located only 3 to 4 light-years from the nebulae and lies just above the right edge of the frame. Slightly closer to gamma Cas, IC 63 is dominated by red H-alpha light emitted as hydrogen atoms ionized by the hot star's ultraviolet radiation recombine with electrons. Farther from the star, IC 59 shows less H-alpha emission but more of the characteristic blue tint of dust reflected star light. The field of view spans over 1 degree or 10 light-years at the estimated distance of the interstellar apparitions.


Image Credit & Copyright: Christophe Vergnes, Hervé Laur

Christophe's website: https://www.astrobin.com/users/Chris.V/

Release Date: Oct. 26, 2024


#NASA #Space #Astronomy #Science #Star #GammaCassiopeiae #GammaCas #Nebulas #Nebulae #IC59 #IC63 #Cassiopeia #MilkyWayGalaxy #Cosmos #Universe #Astrophotographers #ChristopheVergnes #HervéLaur #Astrophotography #STEM #Education #APoD

Wide Field View of Star Gamma Cassiopeia with Nebulae IC 59 & IC 63

Wide Field View of Star Gamma Cassiopeia with Nebulae IC 59 & IC 63

The bright bluish star shown here is Gamma Cassiopeiae. It is currently evaporating two nearby clouds of gas—nebulae IC 59 and IC 63. The leading edges of these clouds glow strongly in the intense bath of radiation from this hot star. Hints of bluish light behind the front lines of these nebulae show a bit of scattered light. Astronomically speaking, these clouds do not have much more time and will soon be blown away into the interstellar medium.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center.


Credit: KPNO/NOIRLab/NSF/AURA/Tom Bash and John Fox/Adam Block

Release Date: June 6, 2014


#NASA #Space #Astronomy #Science #Star #GammaCassiopeiae #GammaCas #Nebulae #Nebula #IC59 #IC63 #Cassiopeia #Constellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #KittPeak #Tucson #Arizona #NOIRLab #AURA #NSF #UnitedStates #STEM #Education

The 'Ghosts' of Star Gamma Cassiopeia: Nebulae IC 59 & IC 63

The 'Ghosts' of Star Gamma CassiopeiaNebulae IC 59 & IC 63

Gamma Cassiopeiae shines high in northern autumn evening skies. It is the brightest spiky star in this telescopic field of view toward the constellation Cassiopeia. Gamma Cas shares the ethereal-looking scene with ghostly interstellar clouds of gas and dust, IC 59 and IC 63. About 600 light-years distant, the clouds are not actually ghosts. They are slowly disappearing though, eroding under the influence of energetic radiation from hot and luminous gamma Cas. Gamma Cas is physically located only 3 to 4 light-years from the nebulae. Slightly closer to gamma Cas, IC 63 is dominated by red H-alpha light emitted as hydrogen atoms ionized by the star's ultraviolet radiation recombine with electrons. Farther from the star, IC 59 shows proportionally less H-alpha emission but more of the characteristic blue tint of dust reflected star light. The cosmic stage spans over 1 degree or 10 light-years at the estimated distance of gamma Cas and friends.

Astrophotographer Markus Horn: "The area around the well-known 'Ghost of Cassiopeia' had been on my agenda for a while, and this year I was finally able to make it happen. Once again, I wanted to use my fast f/2 optics and a 400mm focal length to capture not only RGB data but also as much H-alpha signal as possible across the entire region. My goal was to show how deeply IC 63 and IC 59 are embedded within the H-alpha clouds. For this, I gathered 9.5 hours of RGB and 6.75 hours of H-alpha data."

"To ensure that the beautiful reflection nebulae of IC 63 and IC 59 weren’t completely overwhelmed by the narrowband data, I combined the H-alpha data in this area with the RGB data using continuum substraction. Finally, I invested a few more hours in finding a good balance between the RGB and narrowband components for the final image."

Image Details:
Celestron RASA 8 f/2
Celestron Motorfocus
EQ6-R Pro
ZWO ASI 2600 MC Pro (Gain 100, Offset 18, -10°)
RGB: 576 × 60″ (9h 36′)
TS 2600 MP (Gain 100, Offset 200, -10°)
Baader H-Alpha Highspeed 3.5nm: 202 × 120″ (6h 44')
Total: 16h 20'
Bortle 5 (19.50 SQM)
N.I.N.A., Guiding: ASI 120MM & PHD2
Astropixelprocessor, Photoshop, Pixinsight

Image Credit: Markus Horn
Release Date: Nov. 7, 2024

#NASA #Space #Astronomy #Science #Star #GammaCassiopeiae #GammaCas #Nebulae #Nebula #IC59 #IC63 #Cassiopeia #MilkyWayGalaxy #Cosmos #Universe #Astrophotographer #MarkusHorn #Astrophotography #STEM #Education

Star Trail Photography: Sunset to Sunrise | International Space Station

Star Trail Photography: Sunset to Sunrise | International Space Station

NASA astronaut Don Pettit: "This 30-minute time exposure through orbital night with our new 15mm wide-angle lens was able to capture sunset (on the left) all the way to sunrise (on the right). I have never been able to capture this before but our new fast (14mm f1.4 and 15mm T1.8) wide-angle lenses are opening up observations previously not possible. Visible are circular star trails above the earth limb created not from Earth rotation but from our orbital motion (pitch axis of ISS), cities streaking by (again due to orbital motion), lightning flashes, aurora, atmospheric airglow (both strong green and fainter red). Stay tuned for more of these."

Image details: Nikon Z9, Arri-Zeiss 15mm T1.8 master prime lens, 30 seconds at T1.8 for individual exposures assembled with Photoshop into a composite equivalent to a 30-minute exposure, ISO 200, adjusted for levels, contrast, color, and spot removal. With our current 8-year-old laptops, I cannot perform dark frame subtraction followed by robust denoise operations (would take about 30 hours run time for a single composition where cosmic rays would probably require a re-boot in the process), so clean, finished photographs will have to wait until I return to Earth."

Expedition 72 Updates:

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

Expedition 72 Crew

Station Commander: Suni Williams

Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov

NASA: Butch Wilmore, Don Pettit, Nick Hague

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.


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

Release Date: Nov. 7, 2024


#NASA #Space #Science #ISS #Earth #Astronauts #DonPettit #AstronautPhotography #Timelapse #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education

Aurora Dome over Labrador

Aurora Dome over Labrador


Astrophotographer Adam Woodworth: "During the intense aurora on October 10, 2024, my buddy Steve Sheppard and I experienced the most amazing display of aurora that either of us had ever seen. For most of the night the aurora was clearly visible in the sky but still faint enough that you could barely make out some green color with the naked eye. But at one point the sky exploded with bright colors and we were under a horizon to horizon 360 degree dome of aurora for a few minutes. It was so bright it lit up the ground, and we could clearly see color all across the sky . . ."

Image Details: Nikon Z 6 with Sigma 14mm f/1.8 lens @ f/1.8, ISO 1250, 2 seconds for all exposures in this panorama

Labrador is a geographic region within the Canadian province of Newfoundland and Labrador.

On Earth, auroras are mainly created by particles originally emitted by the Sun in the form of solar wind. When this stream of electrically charged particles gets close to our planet, it interacts with the magnetic field, which acts as a gigantic shield. While it protects Earth’s environment from solar wind particles, it can also trap a small fraction of them. Particles trapped within the magnetosphere—the region of space surrounding Earth in which charged particles are affected by its magnetic field—can be energized and then follow the magnetic field lines down to the magnetic poles. There, they interact with oxygen and nitrogen atoms in the upper layers of the atmosphere, creating the flickering, colorful lights visible in the polar regions here on Earth.

Earth auroras have different names depending on which pole they occur at. Aurora Borealis, or the northern lights, is the name given to auroras around the north pole and Aurora Australis, or the southern lights, is the name given for auroras around the south pole.

Learn more:
The Colors of the Aurora (National Park Service)
https://www.nps.gov/articles/-articles-aps-v8-i1-c9.htm


Image Credit & Copyright: Adam Woodworth
Adam's website: https://www.adamwoodworth.com
Image Date: Oct. 10, 2024
Release Date: Nov. 6, 2024

#NASA #Space #Science #Earth #Planet #Aurora #AuroraBorealis #NorthernLights #MagneticField #Magnetosphere #SolarWind #Sun #Astrophotography #Astrophotographer #AdamWoodworth #Labrador #Newfoundland #Canada #STEM #Education

NASA X-59 Research Aircraft Fires Up its Engine for First Time

NASA X-59 Research Aircraft Fires Up its Engine for First Time

NASA’s X-59 quiet supersonic research aircraft sits in its run stall at Lockheed Martin’s Skunk Works facility in Palmdale, California, firing up its engine for the first time. These engine-run tests start at low power and allow the X-59 team to verify the aircraft’s systems are working together while powered by its own engine. 
Direct view of the front of the X-59 aircraft, mostly in the shade of a run stall. Flaps on both wings are activated, moving downward. Team members wear protective ear guards and look at the aircraft from both sides. NASA’s 100-foot-long X-59 sits in the run stall with the engine and the rest of the back of the aircraft sitting outside the run stall’s open bay door at Lockheed Martin’s Skunk Works facility in Palmdale, California, prior to its first engine run. Engine runs are part of a series of integrated ground tests needed to ensure safe flight and successful achievement of mission goals.
View of an aircraft cockpit inside a run stall. The canopy atop the cockpit is open. Inside, a pilot looks at his instruments as he wears a helmet and oxygen mask. The white, gold, and blue paint scheme of the NASA aircraft is prominent. Lockheed Martin test pilot Dan Canin sits in the cockpit of NASA’s X-59 quiet supersonic research aircraft in a run stall at Lockheed Martin’s Skunk Works facility in Palmdale, California prior to its first engine run.

NASA’s Quesst mission marked a major milestone with the start of tests on the engine that will power the quiet supersonic X-59 experimental aircraft.

These engine-run tests started on Oct. 30, 2024. They allow the X-59 team to verify the aircraft’s systems are working together while powered by its own engine. In previous tests, the X-59 used external sources for power. The engine-run tests set the stage for the next phase of the experimental aircraft’s progress toward flight.

The X-59 team is conducting the engine-run tests in phases. In this first phase, the engine rotated at a relatively low speed without ignition to check for leaks and ensure all systems are communicating properly. The team then fueled the aircraft and began testing the engine at low power, with the goal of verifying that it and other aircraft systems operate without anomalies or leaks while on engine power.

“The first phase of the engine tests was really a warmup to make sure that everything looked good prior to running the engine,” said Jay Brandon, NASA’s X-59 chief engineer. “Then we moved to the actual first engine start. That took the engine out of the preservation mode that it had been in since installation on the aircraft. It was the first check to see that it was operating properly and that all the systems it impacted—hydraulics, electrical system, environmental control systems, etc.—seemed to be working.”

The X-59 will generate a quieter thump rather than a loud boom while flying faster than the speed of sound. The aircraft is the centerpiece of NASA’s Quesst mission. It will gather data on how people perceive these thumps, providing regulators with information that could help lift current bans on commercial supersonic flight over land.

The engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.

Engine runs are part of a series of integrated ground tests needed to ensure safe flight and successful achievement of mission goals. Because of the challenges involved with reaching this critical phase of testing, the X-59’s first flight is now expected in early 2025. The team will continue progressing through critical ground tests and address any technical issues discovered with this one-of-a-kind, experimental aircraft. The X-59 team will have a more specific first flight date as these tests are successfully completed.

The testing is taking place at Lockheed Martin’s Skunk Works facility in Palmdale, California. During later phases, the team will test the aircraft at high power with rapid throttle changes, followed by simulating the conditions of an actual flight.

“The success of these runs will be the start of the culmination of the last eight years of my career,” said Paul Dees, NASA’s deputy propulsion lead for the X-59. “This isn’t the end of the excitement but a small steppingstone to the beginning. It’s like the first note of a symphony, where years of teamwork behind the scenes are now being put to the test to prove our efforts have been effective, and the notes will continue to play a harmonious song to flight.”

After the engine runs, the X-59 team will move to aluminum bird testing, where data will be fed to the aircraft under both normal and failure conditions. The team will then proceed with a series of taxi tests, where the aircraft will be put in motion on the ground. These tests will be followed by final preparations for first flight.

The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.

Learn more here:

https://www.nasa.gov/mission/quesst/

https://www.nasa.gov/flightlog

X-59 Free Maker Bundle (STEM Education):

https://www.nasa.gov/sites/default/files/atoms/files/x-59-maker-bundle-v8.pdf


Image Credit: NASA/Carla Thomas
Article Credit: NASA Langley
Release Date: Nov. 6, 2024


#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #EngineRunTests #FlightTests #LockheedMartin #SkunkWorks #NASAArmstrong #AFRC #California #UnitedStates #STEM #Education

Wednesday, November 06, 2024

NASA "Espacio a Tierra" | Votar desde el espacio : 01 de noviembre de 2024

NASA "Espacio a Tierra" | Votar desde el espacio : 01 de noviembre 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: 4 minute, 21 seconds

Release Date: Nov. 6, 2024


#NASA #Space #Science #ISS #Earth #NASAenespañol #español #USElection #AstronautVoting #SpaceX #CargoDragonSpacecraft #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education #HD #Video

China's Space Exploration Goals: Moon Landing & Mars Sample Return Missions

China's Space Exploration Goals: Moon Landing & Mars Sample Return Missions

China aims to launch a Mars-sample return mission around 2028 and to land taikonauts on the Moon by 2030. From launching its first satellite, Dongfanghong-1, in 1970 to sending the first Chinese taikonaut, Yang Liwei, into space in 2003; from completing the construction of its Tiangong space station in 2022 to collecting lunar samples from the far side of the Moon this year with the Chang'e-6 Mission, China's space exploration has achieved historic leaps. 

For example, China was the first country to successfully send an orbiter, lander and rover to Mars on its first attempt. China is only the second country after the United States to successfully land and operate a spacecraft on Mars.

China's Tianwen-1 Mars probe was launched back in July 2020 and entered Mars orbit in February 2021. The rover landed and started operations in May 2021. After it completed 90 Martian days of assigned scientific exploration tasks, the rover continued its exploration of the Red Planet. The rover, which has traveled 1,921 meters in 358 Martian days, is now in sleep mode.

As of June 29, 2022, the orbiter of the Tianwen-1 mission had completed its primary global remote sensing exploration objectives. It has been in operation for over 1,000 days. It remains in good condition and will continue to conduct scientific exploration and accumulate data from orbit, according to the China National Space Administration (CNSA).


Video Credit: CGTN
Duration: 2 minutes
Release Date: Oct. 1, 2024


#NASA #Space #Astronomy #Science #Mars #Tianwen1 #Moon #Change6 #Earth #China #中国 #LongMarchRockets #Dongfanghong1 #Satellites #Taikonauts #CSS #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceTechnology #Engineering #CMSA #国家航天局 #HumanSpaceflight #Spaceflight #SpaceExploration #SolarSystem #History #STEM #Education #HD #Video

Strong X2.3 Solar Flare Erupts from Sun | NASA’s Solar Dynamics Observatory

Strong X2.3 Solar Flare Erupts from Sun | NASA’s Solar Dynamics Observatory


The Sun emitted a strong solar flare, peaking at 8:40 a.m. ET on Nov. 6, 2024. NASA’s Solar Dynamics Observatory (SDO) watches the Sun constantly and captured images of the event.

Visual Description: A portion of the Sun, shown in red. Toward the middle of the image are bright white and yellow areas. A spurt of solar material erupts from the area.

NASA’s Solar Dynamics Observatory captured this image of a solar flare—seen as the bright flash near the center—on Nov. 6, 2024. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in red. 

Solar flares are powerful bursts of energy. Flares and solar eruptions can impact radio communications, electric power grids, navigation signals, and pose risks to spacecraft and astronauts.

This flare is classified as an X2.3 class flare. X-class denotes the most intense flares, while the number provides more information about its strength.

To see how such space weather may affect Earth, please visit NOAA’s Space Weather Prediction Center https://spaceweather.gov/, the U.S. government’s official source for space weather forecasts, watches, warnings, and alerts. 

NASA works as a research arm of the nation’s space weather effort. NASA observes the Sun and our space environment constantly with a fleet of spacecraft that study everything from the Sun’s activity to the solar atmosphere, and to the particles and magnetic fields in the space surrounding Earth.


Credit: NASA/SDO

Release Date: Nov. 6, 2024


#NASA #Astronomy #Space #Science #Earth #Moon #SpaceWeather #Sun #Star #Solar #SolarFlares #Sunspots #Ultraviolet #Plasma #MagneticField #Astrophysics #Heliophysics #Physics #Spacecraft #Satellites #ElectricalGrids #SDO #SolarSystem #GSFC #UnitedStates #GIF #Animation #STEM #Education

SpaceX Starship Fifth Flight Test Recap & Looking Ahead to The Sixth Flight

SpaceX Starship Fifth Flight Test Recap & Looking Ahead to The Sixth Flight

Starship’s fifth flight test on October 13, 2024, was a "seminal moment in iterating towards a fully and rapidly reusable launch system. The sixth flight test of Starship is targeted to launch as early as Monday, November 18."

For 6th Flight Test updates and the upcoming webcast, visit:

http://spacex.com/launches/mission/?missionId=starship-flight-6

"Starship executed another successful hot-staging separation, igniting its six Raptor engines and completing ascent into outer space. It coasted along its planned trajectory to the other side of the planet before executing a controlled reentry, passing through the phases of peak heating and maximum aerodynamic pressure, before executing a flip, landing burn, and splashdown at its target area in the Indian Ocean. The flight test concluded at splashdown 1 hour, 5 minutes and 40 seconds after launch."

"The entire SpaceX team should take pride in the engineering feat they just accomplished. The world witnessed what the future will look like when Starship starts carrying crew and cargo to destinations on Earth, the Moon, Mars and beyond."

Review the mission summary here:

"Starship is essential to both SpaceX’s plans to deploy its next-generation Starship system as well as for NASA, which will use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis III mission through the Human Landing System (HLS) program."

Key Starship Parameters:

Height: 121m/397ft

Diameter: 9m/29.5ft

Payload to LEO: 100 – 150t (fully reusable)

Download the Free Starship User Guide (PDF):

https://www.spacex.com/media/starship_users_guide_v1.pdf


Video Credit: Space Exploration Technologies Corporation (SpaceX)
Duration: 3 minutes, 28 seconds
Capture Date: Oct. 13, 2024
Release Date: Nov. 6, 2024


#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #Starship #Spacecraft #Starship5 #TestFlight5 #HeavyBooster #SuperHeavyRocket #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #Starbase #Mechazilla #BocaChica #Texas #UnitedStates #STEM #Education #HD #Video

Orbital Sunrise, Spacecraft & Aurora | International Space Station

Spacecraft, Aurora & Orbital Sunrise | International Space Station

The SpaceX Dragon Freedom spacecraft is pictured docked to the space-facing port on the International Space Station's Harmony module.
The unoccupied space-facing port on the International Space Station's Harmony module is pictured several hours before the SpaceX Dragon Freedom spacecraft would relocate there after undocking from Harmony's forward port.
As the International Space Station soared 257 miles above Lake Michigan, NASA astronaut and Expedition 72 Flight Engineer Don Pettit captured this long-exposure photograph of city lights streaking across Earth while a green and red aurora moved through the atmosphere.
As the International Space Station soared 257 miles above northern Mexico, NASA astronaut and Expedition 72 Flight Engineer Don Pettit captured this long-exposure photograph of city lights streaking across Earth while a green atmospheric glow crowned the horizon.
The first rays of an orbital sunrise illuminate Earth's atmosphere in this photograph from the International Space Station as it orbited 269 miles above the Pacific Ocean near Chile's Patagonia coast on the South American continent.

On Tuesday, November 5, 2024, a SpaceX Dragon cargo spacecraft docked to the forward port of the International Space Station’s Harmony module successfully delivering NASA science investigations, supplies, and equipment to the International Space Station. CRS-31 is the fifth flight for this Dragon spacecraft. It previously flew CRS-21, CRS-23, CRS-25, and CRS-28 to the International Space Station. 

The SpaceX Dragon Freedom spacecraft, with Expedition 72 crew members NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore, as well as Roscosmos cosmonaut Aleksandr Gorbunov, autonomously redocked with the space-facing port of the station’s Harmony module on November 3, 2024.

The port relocation freed up Harmony’s forward-facing port for the 31st SpaceX commercial resupply services mission to the International Space Station. This was the fifth port relocation of a Dragon spacecraft with crew aboard following previous moves during the Crew-1, Crew-2, Crew-6, and Crew-8 missions.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

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 Credit: NASA's Johnson Space Center (JSC)
Capture Dates: Oct. 1-Nov. 4, 2024

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Three African Nations Meet in The Sahara Desert | International Space Station

Three African Nations Meet in The Sahara Desert | International Space Station


The borders of three African nations, Libya, Sudan, and Egypt, meet in the eastern portion of the Sahara in this photograph from the International Space Station as it orbited 258 miles above.

The Sahara is the largest hot desert and the third largest desert in the world after Antarctica and the Arctic. Its area of 9,200,000 square kilometers (3,600,000 sq mi) is comparable to the area of China or the United States. The name 'Sahara' is derived from a dialectal Arabic word for "desert", ṣaḥra (صَحَارَى). 

The Sahara covers much of North Africa, excluding the fertile region on the Mediterranean Sea coast, the Atlas Mountains of the Maghreb, and the Nile Valley in Egypt and Sudan. It stretches from the Red Sea in the east and the Mediterranean in the north to the Atlantic Ocean in the west, where the landscape gradually changes from desert to coastal plains. To the south, it is bounded by the Sahel, a belt of semi-arid tropical savanna around the Niger River valley and the Sudan Region of Sub-Saharan Africa.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

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.

Learn more about the important research being operated on Station:
For more information about STEM on Station:
Science, Technology, Engineering, Math (STEM)

Image Credit: NASA's Johnson Space Center (JSC)
Image Date: Oct. 17, 2024
Release Date: Oct. 18, 2024

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Aurora over Scotland

Aurora over Scotland

On Earth, auroras are mainly created by particles originally emitted by the Sun in the form of solar wind. When this stream of electrically charged particles gets close to our planet, it interacts with the magnetic field, which acts as a gigantic shield. While it protects Earth’s environment from solar wind particles, it can also trap a small fraction of them. Particles trapped within the magnetosphere—the region of space surrounding Earth in which charged particles are affected by its magnetic field—can be energized and then follow the magnetic field lines down to the magnetic poles. There, they interact with oxygen and nitrogen atoms in the upper layers of the atmosphere, creating the flickering, colorful lights visible in the polar regions here on Earth.

Earth auroras have different names depending on which pole they occur at. Aurora Borealis, or the northern lights, is the name given to auroras around the north pole and Aurora Australis, or the southern lights, is the name given for auroras around the south pole.

Learn more:
The Colors of the Aurora (National Park Service)
https://www.nps.gov/articles/-articles-aps-v8-i1-c9.htm

Image Credit & Copyright: Alan Tough
Location: Bishopmill, Scotland, United Kingdom
Image Dates: Oct. 26, 2024 


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