Wednesday, November 13, 2024

'Ominous' Dark Nebula SH2-136 in Cepheus: Wide-field view | NOIRLab

'Ominous' Dark Nebula SH2-136 in Cepheus: Wide-field view | NOIRLab


Dark nebula SH2-136 appears to celebrate Halloween all the time. The complex process of star formation has created dust clouds of many shapes and sizes. It is human perception that might identify a "ghoulish creature", on the left side of the image, "chasing humans". SH2-136 is over two light-years across.

Distance: 1,500 light years

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.


Credit: KPNO/NOIRLab/NSF/AURA/Adam Block
Caption Credit: NASA's Goddard Space Flight Center
Release Date: June 13, 2014


#NASA #Astronomy #Space #Science #Nebulae #Nebula #DarkNebula #GhostNebula #Globule   #SH2136 #VdB141 #StellarNursery #Cepheus #Constellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #Arizona #UnitedStates #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

'Ominous' Dark Nebula SH2-136 in Cepheus: Close-up view | NOIRLab

'Ominous' Dark Nebula SH2-136 in Cepheus: Close-up view | NOIRLab

Dark nebula SH2-136 appears to celebrate Halloween all the time. The complex process of star formation has created dust clouds of many shapes and sizes. It is human perception that might identify a "ghoulish creature", on the left side of the image, "chasing humans". SH2-136 is over two light-years across.

Distance: 1,500 light years

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.


Credit: KPNO/NOIRLab/NSF/AURA/Adam Block
Caption Credit: NASA's Goddard Space Flight Center
Release Date: June 13, 2014


#NASA #Astronomy #Space #Science #Nebulae #Nebula #DarkNebula #GhostNebula #Globule   #SH2136 #VdB141 #StellarNursery #Cepheus #Constellation #MilkyWayGalaxy #Cosmos #Universe #KPNO #Arizona #UnitedStates #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Tuesday, November 12, 2024

Dying star "cocooned" in its own gases: NGC 6886 in Sagitta | Hubble

Dying star "cocooned" in its own gases: NGC 6886 in Sagitta | Hubble


Astronomers have used the NASA/European Space Agency Hubble Space Telescope to image the tiny planetary nebula NGC 6886. These celestial objects signal the final death throes of mid-sized stars (up to about eight times the mass of the Sun). When such a star exhausts its supply of hydrogen fuel, the outer layers begin to expand and cool, which creates an envelope of gas and dust that shrouds the dying star. However, the star does not go down without a fight, finding alternative ways to prevent it from collapsing under its own gravity and emerging as a white dwarf. In the process, the star's surface temperature increases and it is eventually hot enough to emit strong ultraviolet radiation and make the cocoon of gas glow as a planetary nebula.

Distance: 11,000 light years

Stellar death is not quick and painless—the planetary nebula stage typically lasts several tens of thousands of years. By studying the elements that are present in the nebula today, astronomers can determine the original chemical make-up of the star. Studies suggest that the star belonging to NGC 6886 may have originally been similar to the Sun, containing similar quantities of carbon, nitrogen and neon, although heavier elements, such as sulphur, were less plentiful.

Keen amateur astronomers with mid-level telescopes will find it a rewarding challenge to track down NGC 6886 in the small constellation of Sagitta. It is tiny, but not particularly faint: high magnification, a good chart, a dark site and averted vision are needed to spot this elusive celestial jewel.

This picture was created by combining images taken using the Wide Field Planetary Camera 2 on Hubble. Filters that let through emission from ionized nitrogen gas (F658N, colored red), ionized oxygen (F502N, colored blue) and a broadband yellow filter (F555W, colored green, and also contributing to the blue) were used. The exposure times were 700 s, 600 s and 320 s respectively. The field of view is merely 30 arcseconds across.


Credit: ESA/Hubble & NASA
Release Date: Jan. 10, 2011


#NASA #ESA #Astronomy #Space #Science #Hubble #CatsEyeNebula #Nebula #PlanetaryNebula #NGC6886 #Sagitta #Constellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Trimethyl Aluminum Clouds over Norway | NASA Earth Science

Trimethyl Aluminum Clouds over Norway | NASA Earth Science

These clouds are completely harmless, NASA's Goddard Space Flight Center reports. Twisting clouds of trimethyl aluminum (TMA) appeared over Norway on Nov. 10, 2024, during a minor geomagnetic storm. Ivar Sandland photographed them from Narvik, a small town inside the Arctic Circle. Moments earlier, Sandland watched a rocket climb through colorful auroras. "It was a rocket launch from Andoya Space Center in northern Norway," he explains. "Moments later, the clouds appeared."

NASA's rocket carried 16 canisters of trimethyl aluminum. These were released into the upper atmosphere. Glowing clouds were visible from the ground, allowing researchers to study waves and vortices in air ~100 km above Earth's surface—a region which also contains the turbopause. This is fundamental research that may help improve computer models of our planet's atmosphere.

The turbopause, also called the homopause, marks the altitude in an atmosphere below which turbulent mixing dominates.

Earth's turbopause lies near the mesopause, at the intersection of the mesosphere and the thermosphere, at an altitude of roughly 90 km (56 mi). Other turbopauses in the Solar System that are known include Venus' turbopause at about 130–135 km (81–84 mi), Mars' at about 130 km (81 mi), Jupiter's at roughly 385 km (239 mi), and Titan's at around 800–850 km (500–530 mi). 

Earth's turbopause was discovered by French scientists following the firing of two Véronique sounding rockets on March 10 and 12, 1959.


Image Credit: Ivar Sandland
Caption Credit: SpaceWeather[dot]com
Image Date: Nov. 10, 2024
Release Date: Nov. 12, 2024


#NASA #Astronomy #Space #Science #Star #Sun #Heliophysics #SolarSystem #Earth #Atmosphere #Turbopause #AndoyaSpaceport #Narvik #ArcticCircle #Norway #Norge #SoundingRocket #RocketLaunch #SuborbitalFlight #TMAClouds #Aurora #AuroraBorealis #NorthernLights #GSFC #WFF #UnitedStates #STEM #Education

Mining Old Data from NASA’s Voyager 2 Solves Several Uranus Mysteries | JPL

Mining Old Data from NASA’s Voyager 2 Solves Several Uranus Mysteries | JPL

NASA’s Voyager 2 captured this image of planet Uranus while flying by the ice giant in 1986. New research using data from the mission shows a solar wind event took place during the flyby, leading to a mystery about the planet’s magnetosphere that may now be better understood.
Artist’s concept depicts how Uranus’s magnetosphere was acting before and during the flyby of NASA’s Voyager 2. The first panel of this artist’s concept depicts how Uranus’s magnetosphere—its "protective bubble"—was before the flyby of NASA’s Voyager 2. The second panel shows an unusual kind of solar weather was happening during the 1986 flyby, giving scientists a skewed view of the magnetosphere.

NASA’s Voyager 2 spacecraft flyby of Uranus thirty-eight years ago in 1986 shaped scientists’ understanding of the planet but also introduced unexplained oddities. A recent data investigation has offered potential new answers.

NASA’s Voyager 2 spacecraft provided scientists’ first—and, so far, only—close glimpse of this strange, sideways-rotating outer planet. Alongside the discovery of new moons and rings, new mysteries confronted scientists. The energized particles around the planet defied their understanding of how magnetic fields work to trap particle radiation, and Uranus earned a reputation as an outlier in our solar system.

Now, new research analyzing the data collected during that flyby 38 years ago has found that the source of that particular mystery is a cosmic coincidence. It turns out that in the days just before Voyager 2’s flyby, the planet had been affected by an unusual kind of space weather that compressed the planet’s magnetic field substantially. 

“If Voyager 2 had arrived just a few days earlier, it would have observed a completely different magnetosphere at Uranus,” said Jamie Jasinski of NASA’s Jet Propulsion Laboratory (JPL) in Southern California and lead author of the new work published in Nature Astronomy. “The spacecraft saw Uranus in conditions that only occur about 4% of the time.”

Magnetospheres act as "protective bubbles" around planets (including Earth) with magnetic cores and magnetic fields, shielding them from jets of ionized gas—or plasma—that stream out from the Sun in the solar wind. Learning more about how magnetospheres work is also important for understanding our own planet.

Inside Uranus’ magnetosphere were electron radiation belts with an intensity second only to Jupiter’s notoriously brutal radiation belts. However, there was apparently no source of energized particles to feed those active belts. In fact, the rest of Uranus’ magnetosphere was almost devoid of plasma.

The missing plasma also puzzled scientists because they knew that the five major Uranian moons in the magnetic bubble should have produced water ions, as icy moons around other outer planets do. They concluded that the moons must be inert with no ongoing activity.


Solving the Mystery

Why was no plasma observed, and what was happening to boost the radiation belts? The new data analysis points to the solar wind. When plasma from the Sun pounded and compressed the magnetosphere, it likely drove plasma out of the system. The solar wind event also would have briefly intensified the dynamics of the magnetosphere. This would have fed the belts by injecting electrons into them.

The findings could be good news for those five major moons of Uranus. Several of them may be geologically active after all. With an explanation for the temporarily missing plasma, researchers say it is plausible that the moons actually may have been spewing ions into the surrounding bubble all along.

Planetary scientists are focusing on bolstering their knowledge about the mysterious Uranus system. The National Academies’ 2023 Planetary Science and Astrobiology Decadal Survey prioritized it as a target for future NASA missions.

JPL’s Linda Spilker was among the Voyager 2 mission scientists concentrating on the images and other data that arrived during the Uranus flyby in 1986. She remembers the anticipation and excitement of the event. It changed how scientists thought about the Uranian system.

“The flyby was packed with surprises, and we were searching for an explanation of its unusual behavior. The magnetosphere Voyager 2 measured was only a snapshot in time,” said Spilker, who has returned to the iconic mission to lead its science team as project scientist. “This new work explains some of the apparent contradictions, and it will change our view of Uranus once again.”

Voyager 2, now in interstellar space, is almost 13 billion miles (21 billion kilometers) from Earth.


Credits: NASA's Jet Propulsion Laboratory-Caltech
Release Date: Nov. 11, 2024


#NASA #Space #Astronomy #Science #Sun #SolarSystem #SolarWind #Planet #Uranus #Moons #MagneticField #Atmosphere #Voyager2Mission #Voyager2 #Voyager2Spacecraft #InterplanetarySpacecraft #UranusSystemFlyby #JPL #Caltech #UnitedStates #Art #Infographic #STEM #Education

New GOES-19 Satellite Captures Extended Images of Sun's Atmosphere | NOAA

New GOES-19 Satellite Captures Extended Images of Sun's Atmosphere | NOAA 

The National Oceanic and Atmospheric Administration (NOAA) recently unveiled the first images from the Compact Coronagraph (CCOR-1) and the Solar Ultraviolet Imager (SUVI). These are two advanced instruments onboard the NOAA's new GOES-19 satellite, launched on June 25, 2024. These tools are set to "revolutionize" space weather monitoring and forecasting as they begin observing the Sun and its influence on Earth. 

CCOR-1 is the world’s first dedicated operational space-based coronagraph. Using an occulting disk to block the bright surface of the sun, CCOR-1 provides images of the corona every 15 minutes. This powerful telescope is designed to detect and analyze coronal mass ejections (CMEs)—massive bursts of solar plasma and magnetic fields that can significantly impact Earth's space environment. By observing the Sun in the extreme ultraviolet part of the spectrum, SUVI captures phenomena like flares and coronal loop—critical to understanding hazardous space weather.

Note: Data from GOES-19, during its post-launch testing phase, should be considered preliminary and non-operational.

Learn More: https://www.nesdis.noaa.gov/news/noaas-goes-19-captures-extended-images-of-the-suns-atmosphere


Video Credit: National Oceanic and Atmospheric Administration (NOAA)
Duration: 2 minutes
Release Date: Nov. 12, 2024

#NASA #NOAA #Science #Astronomy #Stars #Sun #SolarSystem #Planet #Earth #Satellites #GOES19 #Coronograph #CCOR1 #SolarUltravioletImager #SUVI #SpaceWeather #SolarFlares #Heliophysics #GSFC #UnitedStates #STEM #Education #HD #Video

Sandy Sculptures in Morocco’s Erg Chebbi | International Space Station

Sandy Sculptures in Morocco’s Erg Chebbi | International Space Station

Windswept sand formations known as star dunes, or pyramid dunes, are a distinctive feature of the Sahara Desert in northern Africa. An astronaut aboard the International Space Station took this photograph while orbiting over northern Africa. The image shows a dune field known as Erg Chebbi, located in southeastern Morocco, near the border with Algeria and northeast of the Little Atlas mountain range. This erg, a wide sandy area covered with dunes, lies in the northwestern region of the Sahara Desert.

Dunes are created when the wind transports and deposits fine sand, forming mounds of sediment. The dunes in this photo display multiple smooth sides, known as slip faces, where sand has cascaded down from the peak. The windward side, located on the opposite side from the slip face, is where the wind blows material upward. The dune continues to grow vertically as long as sediment is available and the wind is strong enough to transport it upward. The large dunes crossing the center of the image, characterized by sharp multidirectional ridges, are star dunes. These are also known as pyramid dunes and are a distinctive feature of the Sahara.

The town of Marzouga and nearby communities appear at the bottom right of the image. A large, natural aquifer supports palm groves as well as crops in this arid region. Agricultural fields are the long linear features visible in the image’s bottom right corner.

Tourism provides an additional source of income for the communities due to their proximity to the Erg Chebbi dunes. Road lines, mainly created by off-road vehicles, are visible at the top of the image. Tent camps are located on the east side of the dune field, visible from space as small clusters of light-colored rectangular shapes. These camps are mostly used by tourists, though some of them could represent settlements of the Indigenous Amazigh (Berber) peoples.

Morocco, officially the Kingdom of Morocco, is a country in the Maghreb region of North Africa. It overlooks the Mediterranean Sea to the north and the Atlantic Ocean to the west, and has land borders with Algeria to the east, and the disputed territory of Western Sahara to the south.

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.

Astronaut photograph ISS070-E-105480 was acquired on December 21, 2023, with a Nikon D5 digital camera using a focal length of 1,200 millimeters. It is provided by the ISS Crew Earth Observations Facility and the Earth Science and Remote Sensing Unit at Johnson Space Center.


Image Credit: NASA's Johnson Space Center (JSC)
Article Credit: Wilfredo García López/Jacobs-JETS II Contract/NASA-JSC
Image Date: Dec. 21, 2023
Release Date: Nov. 10, 2024


#NASA #Space #Science #ISS #Earth #Africa #ErgChebbi #Marzouga #Morocco #Ergs #SandDunes #SaharaDesert #Sahara #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #JSC #Houston #Texas #UnitedStates #Expedition70 #STEM #Education المملكة المغربية 

China's Haolong Reusable Cargo Spacecraft Design Demo | China Space Station

China's Haolong Reusable Cargo Spacecraft Design Demo | China Space Station

At the annual Zhuhai Air Show in China being held between November 12-17, 2024, state-owned Aviation Industry Corporation of China (AVIC) displayed a model of its "Haolong" cargo spaceplane under development. It is a reusable spacecraft with rotating wings and a docking port, designed for low-cost space station cargo missions. It has a large wingspan and high lift-to-drag ratio. 

This animation video by Chengdu Aerospace Corporation, a subsidiary of AVIC, demonstrates Haolong's launch, docking, and Earth return capabilities. The Haolong cargo spacecraft's model dimensions: length 10 meters (32 feet) and width 8 meters (26 feet). Chief designer Fang Yuanpeng: "The Haolong cargo spacecraft is a winged configuration aircraft with a high aspect ratio wing layout and a blunt body fuselage with a large swept-back triangular tail."


Video Credit: CMG/CNSA Watcher
Duration: 1 minute, 17 seconds
Release Date: Nov. 11, 2024


#NASA #Space #Science #Earth #China #中国 #CargoSpacecraft #ReusableSpacecraft #Prototype #SpaceTechnology #Haolong #昊龙货运航天飞机 #AVIC #ZhuhaiAirshow #Taikonauts #Astronauts #CSS #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #LongDurationSpaceflight #CMSA #国家航天局 #HumanSpaceflight #STEM #Education #Animation #HD #Video

Star Trail Oval Art | International Space Station

Star Trail Oval Art | International Space Station

NASA astronaut Don Pettit: "Star trail out forward looking window. When observing Earth, I like the effect of an oval window. It adds a certain measure of aesthetics over that of a round window. However, when you are living in a metal can for six months at a time, I will be happy with any shape of window."

Image Details: Nikon Z9, 8mm fisheye, 30 second exposures at f2.8, ISO 640, assembled in Photoshop to make an effective 30 minute time exposure.

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 #StarTrails #Timelapse #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #Art #STEM #Education

Monday, November 11, 2024

¿Cómo puedo trabajar en la NASA? Preguntamos a un experto de la NASA

¿Cómo puedo trabajar en la NASA? Preguntamos a un experto de la NASA

¡Hay muchas maneras de trabajar en la NASA! No solo necesitamos ingenieros, científicos y astronautas, también necesitamos a muchos otros profesionistas como historiadores, comunicólogos, abogados, artistas y muchos otros oficios. Andrés Almeida, escritor técnico de la NASA, te explica cómo hay diferentes caminos para llegar a la agencia, desde pasantías a oportunidades a través de nuestros sitios web de empleo.

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

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: https://www.nasa.gov/suscribete


Crédito de video: NASA 360
Duration: 1 minute
Release Date: Nov 11, 2024


#NASA #Space #Astronomy #Science #NASAenespañol #español #Trabajar #Students #Professionals #Jobs #Careers #USAJobs #UnitedStates #STEM #Education #HD #Video

A Globular Star Cluster Collection

A Globular Star Cluster Collection

This collage shows a range of globular clusters that were studied using the Hubble Space Telescope and the MPG/ESO 2.2-meter telescope at the European Southern Observatory's La Silla Observatory in Chile. The data show that, despite all forming at roughly the same time, the clusters have aged at dramatically different rates with heavier stars sinking to the centers of the clusters in a process similar to sedimentation.

Top row: Messier 4 (ESO), Omega Centauri (ESO), Messier 80 (Hubble)
Middle row: Messier 53 (Hubble), NGC 6752 (Hubble), Messier 13 (Hubble)
Bottom row: Messier 4 (Hubble), NGC 288 (Hubble), 47 Tucanae (Hubble)


Image Credits:
M 4: European Southern Observatory
Omega Cen: ESO/INAF-VST/OmegaCAM
M 80: The Hubble Heritage Team (AURA/STScI/NASA/ESA)
M 53: ESA/Hubble & NASA
NGC 6752: ESA/Hubble & NASA
M 13: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
M 4: ESA/Hubble & NASA
NGC 288: ESA/Hubble & NASA
47 Tucanae: NASA, ESA, and G. Meylan (École Polytechnique Federale de Lausanne)

Release Date: Dec. 19, 2012


#NASA #ESA #ESO #Astronomy #Space #Science #Stars #StarClusters #GlobularStarClusters #HubbleSpaceTelescope #HST #Cosmos #Universe #Europe #GSFC #STScI #UnitedStates #LaSillaObservatory #Chile #Infographic #STEM #Education

Globular Star Cluster M13 in Hercules: The 'Snow Globe' | Hubble

Globular Star Cluster M13 in Hercules: The 'Snow Globe' | Hubble


Like a whirl of shiny flakes sparkling in a snow globe, the NASA/European Space Agency Hubble Space Telescope caught an instantaneous glimpse of many hundreds of thousands of stars moving about in the globular cluster Messier 13 (M13)—one of the brightest and best-known globular clusters in the northern sky. This glittering metropolis of stars is easily found in the winter sky in the constellation Hercules and can even be glimpsed with the unaided eye under dark skies.

M13 is home to over 100,000 stars and located at a distance of 25,000 light-years. These stars are packed so closely together in a ball, approximately 150 light-years across, that they will spend their entire lives whirling around in the cluster.

This image is a composite of archival Hubble data taken with the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys. Observations from four separate science proposals taken in November 1999, April 2000, August 2005, and April 2006 were used. The image includes broadband filters that isolate light from the blue, visible, and infrared portions of the spectrum.


Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

Release Date: Dec. 4, 2008


#NASA #ESA #Astronomy #Space #Science #StarClusters #GlobularStarClusters #Messier13 #M13 #NGC6205 #GreatHerculesCluster #GreatGlobularCluster #Galaxy #NGC6207 #Hercules #Constellation #HubbleSpaceTelescope #HST #Cosmos #Universe #Europe #GSFC #STScI #UnitedStates #STEM #Education

The Great Globular Star Cluster Messier 13 in Hercules: Wide-field view

The Great Globular Star Cluster Messier 13 in Hercules: Wide-field view

In 1716, English astronomer Edmond Halley noted, "This is but a little Patch, but it shows itself to the naked Eye, when the Sky is serene and the Moon absent." Of course, M13 is now less modestly recognized as the Great Globular Cluster in Hercules—one of the brightest globular star clusters in the northern sky.

Sharp telescopic views like this one reveal the spectacular cluster's hundreds of thousands of stars. At a distance of 25,000 light-years, the cluster stars crowd into a region 150 light-years in diameter. Approaching the cluster core, upwards of 100 stars could be contained in a cube just 3 light-years on a side. For comparison, the closest star to the Sun is over 4 light-years away. The deep, wide-field image also reveals distant background galaxies including NGC 6207 at the upper left, and faint, foreground Milky Way dust clouds known to some as integrated flux nebulae.

In 1974, the former United States Arecibo Observatory, a radio telescope in Puerto Rico, sent a message containing encoded information about humans, DNA, atomic numbers, Earth's position and other information, towards Messier 13 as an experiment in contacting potential extraterrestrial civilizations in the cluster. M13 was chosen because it was a large, relatively close star cluster that was available at the time. The cluster will move through space during the transit time; views differ on whether the cluster will be in a position to receive the message by the time that it arrives in ~25,000 years. Arecibo was the world's largest radio telescope for over half a century— from its construction in 1963 until 2016. Today, the Square Kilometre Array (SKA) in Australia holds that record.


Image Credit & Copyright: Jan Beckmann, Julian Zoller, Lukas Eisert, Wolfgang Hummel
Astrophotographer Team Website:
Caption Credit: NASA Goddard
Release Date: Sept. 26, 2024


#NASA #Astronomy #Space #Science #StarClusters #GlobularStarClusters #Messier13 #M13 #GreatHerculesCluster #GreatGlobularCluster #Galaxy #NGC6207 #Hercules #Constellation #Astrophotography #Astrophotographers #DistantLuminosity #CitizenScience #GSFC #UnitedStates #STEM #Education #APoD

Crowded Heart of The Hercules Globular Star Cluster | Hubble Space Telescope

Crowded Heart of The Hercules Globular Star Cluster | Hubble Space Telescope

This image, taken by the Advanced Camera for Surveys on the Hubble Space Telescope, shows the core of the great globular cluster Messier 13 and provides an extraordinarily clear view of the hundreds of thousands of stars in the cluster—one of the brightest and best known in the sky. Just 25,000 light-years away and about 145 light-years in diameter, Messier 13 has drawn the eye since its discovery by Edmund Halley, the noted British astronomer, in 1714. The cluster lies in the constellation of Hercules and is so bright that under the right conditions it is even visible to the unaided eye. As Halley wrote: “This is but a little Patch, but it shews it self to the naked Eye, when the Sky is serene and the Moon absent.” Messier 13 was the target of a symbolic Arecibo radio telescope message that was sent in 1974, communicating humanity’s existence to possible extraterrestrial intelligences. However, more recent studies suggest that planets are very rare in the dense environments of globular clusters.

Messier 13 has also appeared in literature. In his 1959 novel, The Sirens of Titan, Kurt Vonnegut wrote “Every passing hour brings the Solar System forty-three thousand miles closer to Globular Cluster M13 in Hercules—and still there are some misfits who insist that there is no such thing as progress.” The step from Halley’s early telescopic view to this Hubble image indicates the progress in astronomy over the last three hundred years.

This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys on the Hubble Space Telescope. Data through a blue filter (F435W) are colored blue, data through a red filter (F625W) are colored green and near-infrared data (through the F814W filter) are colored red. The exposure times are 1480 s, 380 s and 567 s respectively and the field of view is about 2.5 arcminutes across.


Credit: ESA/Hubble and NASA
Release Date: July 5, 2010


#NASA #ESA #Astronomy #Space #Science #StarClusters #GlobularStarClusters #Messier13 #M13 #GreatHerculesCluster #GreatGlobularCluster #Galaxy #NGC6207 #Hercules #Constellation #HubbleSpaceTelescope #HST #Cosmos #Universe #Europe #GSFC #STScI #UnitedStates #STEM #Education

Hawaiian Night Skyline from Maunakea | Gemini North Telescope

Hawaiian Night Skyline from Maunakea | Gemini North Telescope


The starry band of our Milky Way galaxy hangs overhead in this panorama taken from Maunakea, the home of Gemini North, one half of the International Gemini Observatory, supported in part by the U.S. National Science Foundation (NSF) and operated by NOIRLab. Down on the mountain at the center of the image, a snaking band of light marks the location of an access road. In the distance, large cities on the Island of Hawai‘i light up spots under the clouds while the active volcano Mauna Loa rises above them.

Just like Mauna Loa, Maunakea is a shield volcano—though thankfully a dormant one. However, the volcanic past of Maunakea continues to be an asset to astronomers. The mountain’s smoothly sloping sides and high elevation are two of the factors that contribute to the exceptional observing conditions at the summit.

The 8.1-meter diameter optical/infrared North Gemini Telescope is located on Hawaii‘s Maunakea as part of the international community of observatories built to take advantage of the superb atmospheric conditions on this long-dormant volcano that rises about 4,214 meters (13,825 feet) into the dry, stable air of the Pacific. The Gemini Observatory's international headquarters is located in Hilo, Hawai‘i at the University of Hawaii Hilo's University Park. 

Since 2002 Gemini North has also been known as the Frederick C. Gillett Gemini North telescope. Dr. Gillett, who died in April 2001, was one of the primary visionaries of the Gemini telescopes. He was instrumental in assuring that the design of Gemini's twin 8-meter telescopes would make major scientific contributions to astronomy.

Learn more about Gemini North here: https://www.gemini.edu


Image Credit: International Gemini Observatory / NOIRLab / NSF / AURA / J. Chu 
Release Date: Nov. 6, 2024

#NASA #Astronomy #Space #Science #Stars #MilkyWayGalaxy #SolarSystem #Cosmos #Universe #LightPollution #InternationalGeminiObservatory #GeminiNorthTelescope #Optical #NOIRLab #AURA #NSF #MaunaLoa #Maunakea #Hawaii #UnitedStates #STEM #Education

The Rosetta Mission: How the European Space Agency Landed on a Comet

The Rosetta Mission: How the European Space Agency Landed on a Comet

On November 12, 2014, after a ten-year journey through the Solar System and over 500 million kilometers from home, Rosetta’s lander Philae made space exploration history by touching down on a comet for the first time. On the occasion of the tenth anniversary of this extraordinary feat, we celebrate by taking a look back over the mission's highlights.

Rosetta was a European Space Agency mission with contributions from its Member States and NASA. It studied Comet 67P/Churyumov-Gerasimenko for over two years, including delivering lander Philae to the comet’s surface. Philae was provided by a consortium led by the German Aeropace Center (DLR), the Max Planck Institute for Solar System Research (MPS), France's Centre national d'études spatiales (CNES) and Italy's Agenzia Spaziale Italiana (ASI).

Learn more about ESA's historic Rosetta Mission:

https://www.esa.int/Science_Exploration/Space_Science/Rosetta/Mission_complete_Rosetta_s_journey_ends_in_daring_descent_to_comet


Credit: ESA - European Space Agency
Duration: 9 minutes
Release Date: Nov. 11, 2024


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