Thursday, November 07, 2024

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

#NASA #Space #Science #ISS #Sun #SolarSystem #Earth #Canadarm2 #SpaceXDragonFreedom #Aurora #OrbitalSunrise #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #Florida #UnitedStates #Expedition72 #STEM #Education

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

#NASA #Space #Science #ISS #Earth #Africa #SaharaDesert #Sahara #Libya #Sudan #Egypt #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #Florida #UnitedStates #Expedition72 #STEM #Education

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 


#NASA #Space #Science #Earth #Planet #Aurora #AuroraBorealis #NorthernLights #MagneticField #Magnetosphere #SolarWind #Sun #Astrophotography #Astrophotographer #AlanTough #Bishopmill #Scotland #UK #UnitedKingdom #STEM #Education

Trapezium Star Cluster in The Orion Nebula | Hubble Space Telescope

Trapezium Star Cluster in The Orion Nebula | Hubble Space Telescope


Appearing like glistening precious stones, the Trapezium cluster's central region is here seen through the eyes of the NASA/European Space Agency Hubble Space Telescope. All of the celestial objects in the Trapezium were born together in this hotbed of star formation. The cluster is named for the trapezoidal alignment of those central massive stars.

Probing deep within a neighborhood stellar nursery, the Hubble Space Telescope uncovered a swarm of newborn brown dwarfs. The orbiting observatory's near-infrared camera revealed about 50 of these objects throughout the Orion Nebula's Trapezium cluster about 1,500 light-years from Earth.

This stellar nursery, Messier 42, popularly called the Orion Nebula, has been known to many cultures throughout human history. The nebula is only 1,500 light-years away, making it the closest large star-forming region to Earth and giving it a relatively bright apparent magnitude of 4. Because of its brightness and prominent location just below Orion’s belt, M42 can be spotted with the naked eye, while offering an excellent peek at stellar birth for those with telescopes. It is best observed during January.


Credit: K.L. Luhman (Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.); and G. Schneider, E. Young, G. Rieke, A. Cotera, H. Chen, M. Rieke, R. Thompson (Steward Observatory, University of Arizona, Tucson, Ariz.) and NASA/ESA

Release Date: August 24, 2000


#NASA #ESA #Astronomy #Space #Hubble #Nebulae #Nebula #OrionNebula #Messier42 #Messier43 #Stars #TrapeziumStars #TrapeziumCluster #BrownDwarfs #Orion #Constellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education

Tuesday, November 05, 2024

Journey to The Orion Nebula | Hubble Space Telescope

Journey to The Orion Nebula | Hubble Space Telescope

This sequence zooms on three ground-based images and ends up with a Hubble image of Messier 42 (M42)—the Orion Nebula. Packed into the center of this region are bright lights of the Trapezium stars, the four heftiest stars in the Orion Nebula. Ultraviolet light unleashed by these stars is carving a cavity in the nebula and disrupting the growth of hundreds of smaller stars. 

Distance: 1,500 light years

This stellar nursery, Messier 42, popularly called the Orion Nebula, has been known to many cultures throughout human history. The nebula is only 1,500 light-years away, making it the closest large star-forming region to Earth and giving it a relatively bright apparent magnitude of 4. Because of its brightness and prominent location just below Orion’s belt, M42 can be spotted with the naked eye, while offering an excellent peek at stellar birth for those with telescopes. It is best observed during January.


Credit: NASA, European Space Agency, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team

Duration: 2 minutes

Release Date: Jan. 11, 2006


#NASA #ESA #Astronomy #Space #Hubble #Nebulae #Nebula #OrionNebula #Messier42 #Messier43 #Stars #TrapeziumStars #UltravioletLight #Orion #Constellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #SD #Video

The Orion Nebula's Largest & Brightest Stars | Hubble Space Telescope

The Orion Nebula's Largest & Brightest Stars | Hubble Space Telescope

Packed into the center of this region are bright lights of the Trapezium stars, the four heftiest stars in the Orion Nebula. Ultraviolet light unleashed by these stars is carving a cavity in the nebula and disrupting the growth of hundreds of smaller stars. The dark speck near the bottom, right of the image is a silhouette of an edge-on disk encircling a young star. Another whitish-looking disk is visible near the bottom, left, just above the two bright stars. This disk is encased in a bubble of gas and dust.

Distance: 1,500 light years

This stellar nursery, Messier 42, popularly called the Orion Nebula, has been known to many cultures throughout human history. The nebula is only 1,500 light-years away, making it the closest large star-forming region to Earth and giving it a relatively bright apparent magnitude of 4. Because of its brightness and prominent location just below Orion’s belt, M42 can be spotted with the naked eye, while offering an excellent peek at stellar birth for those with telescopes. It is best observed during January.


Credit: NASA, European Space Agency, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team

Release Date: Jan. 11, 2006


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Nebula IRAS 05437+2502 in Taurus | Hubble Space Telescope

Nebula IRAS 05437+2502 in Taurus | Hubble Space Telescope

The little-known nebula IRAS 05437+2502 billows out among the bright stars and dark dust clouds that surround it in this striking image from the Hubble Space Telescope. It is located in the constellation of Taurus (the Bull), close to the central plane of our Milky Way galaxy. Unlike many of Hubble’s targets, this object has not been studied in detail and its exact nature is unclear. 

At first glance it appears to be a small, rather isolated, region of star formation and one might assume that the effects of fierce ultraviolet radiation from bright young stars probably were the cause of the eye-catching shapes of the gas. However, the bright boomerang-shaped feature may tell a more dramatic tale. The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp-edged bright arc. Such a reckless star would have been ejected from the distant young cluster where it was born and would travel at 200,000 km/hour or more through the nebula.

This faint cloud was originally discovered in 1983 by the Infrared Astronomical Satellite (IRAS), the first space telescope to survey the whole sky in the infrared. IRAS was run by the United States, the Netherlands, and the United Kingdom and found huge numbers of new objects that were invisible from the ground.

This image was taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. It was part of a “snapshot” survey. These are lists of observations that are fitted into Hubble’s busy schedule when possible. 

This picture was created from images taken through yellow (F606W) and near-infrared (F814W) filters. The exposure times were about eleven minutes per filter and the field of view is about 100 arcseconds across.


Credit: European Space Agency (ESA)/Hubble, R. Sahai and NASA

Release Date: June 14, 2010


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