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This is a frame of old data, left unprocessed.
Tarantula Nebula is in Large Magellanic Cloud, and the distance is about 50kpc or 160kly. It is bright, about mag.8. If it were at the distance as Great Orion Nebula, about 412pc, Tarantula Nebula would have been brighter than now by 150k times, around mag. -7, far brighter than the brightest Venus or the same as 4-day moon.
equipment: Takahashi FSQ-106ED, F3 Reducer 0.6x, and EOS R6-SP5, modified by Seo-san on ZWO AM5 equatorial mount on the genuine tripod with counter weight 4.8kg, autoguided with Fujinon 1:2.8/75mm C-Mount Lens, ZWO ASI 120MM-mini, and PHD2 Guiding
exposure: 4 times x 900 seconds, 3 x 240 sec, 5 x 60 sec, 3 x 15 sec, and 4 x 4 seconds at ISO 1,600 and f/3.0
site: 2,434m above sea level at lat. 24 39 52 south and long. 70 16 11 west near Cerro Armazones in Sierra Vicuña Mackenna in Coast Range of Chile
Ambient temperature was around 10 degrees Celsius or 34 degrees Fahrenheit. Wind was mild. Sky was dark, and SQML reached 21.83 at the night.
The star-forming region, 30 Doradus, is one of the largest located close to the Milky Way and is found in the neighboring galaxy Large Magellanic Cloud. About 2,400 massive stars in the center of 30 Doradus, also known as the Tarantula Nebula, are producing intense radiation and powerful winds as they blow off material.
Multimillion-degree gas detected in X-rays (blue) by the Chandra X-ray Observatory comes from shock fronts -- similar to sonic booms --formed by these stellar winds and by supernova explosions. This hot gas carves out gigantic bubbles in the surrounding cooler gas and dust shown here in infrared emission from the Spitzer Space Telescope (orange).
30 Doradus is also known as an HII (pronounced "H-two") region, created when the radiation from hot, young stars strips away the electrons from neutral hydrogen atoms (HI) to form clouds of ionized hydrogen (HII). It is the most massive and largest HII region in the Local Group of galaxies, which contains the Milky Way, Andromeda and about 30 other smaller galaxies including the two Magellanic Clouds. Because of its proximity and size, 30 Doradus is an excellent target for studying the effects of massive stars on the evolution of an HII region.
The Tarantula Nebula is expanding, and researchers have recently published two studies that attempt to determine what drives this growth. The most recent study concluded that the evolution and the large-scale structure of 30 Doradus is determined by the bubbles of hot, X-ray bright gas confined by surrounding gas, and that pressure from radiation generated by massive stars does not currently play an important role in shaping the overall structure. A study published earlier in 2011 came to the opposite conclusion and argued that radiation pressure is more important than pressure from hot gas in driving the evolution of 30 Doradus, especially in the central regions near the massive stars. More detailed analysis and deeper Chandra observations of 30 Doradus may help decide between these different ideas.
Credit: X-ray: NASA/CXC/PSU/L. Townsley et al.; Infrared: NASA/JPL/PSU/L. Townsley et al.
Read entire caption/view more images: chandra.harvard.edu/photo/2011/30dor/
Caption credit: Harvard-Smithsonian Center for Astrophysics
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p.s. You can see all of our Chandra photos in the Chandra Group in Flickr at: www.flickr.com/groups/chandranasa/ We'd love to have you as a member!
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The Tarantula & Dragon Face nebula region of the Large Magellanic Cloud (LMC).
The LMC is a companion satellite galaxy of our Milkyway 163,000LY away and only visible from the southern hemisphere.
Taken through a 8" SCT at f1.9 with a Hyperstar reducer using a QHY268M camera, in RGB natural colour, with added H-Alpha & OIII narrowband signal to emphasize the fainter, more subtle, nebulosity.
Guided with an 80mm refractor at 500mm FL and tracked on a hypertuned CGEM mount.
The total integration time for this photo was only 14 hours and 45 minutes.
Glowing brightly about 160 000 light-years away, the Tarantula Nebula is the most spectacular feature of the Large Magellanic Cloud, a satellite galaxy to our Milky Way. This image from VLT Survey Telescope at ESOâs Paranal Observatory in Chile shows the region and its rich surroundings in great detail. It reveals a cosmic landscape of star clusters, glowing gas clouds and the scattered remains of supernova explosions.
More information: www.eso.org/public/images/eso1816a/
Credit:
ESO
This image shows a region of space called LHA 120-N150.
More information: spacetelescope.org/news/heic2004/
Credit: ESA/Hubble, NASA, I. Stephens
A snapshot of the Tarantula Nebula (also known as 30 Doradus) is featured in this image from the NASA/ESA Hubble Space Telescope. The Tarantula Nebula is a large star-forming region of ionized hydrogen gas that lies 161,000 light-years from Earth in the Large Magellanic Cloud, and its turbulent clouds of gas and dust appear to swirl between the region’s bright, newly formed stars.
The Tarantula Nebula is a familiar site for Hubble. It is the brightest star-forming region in our galactic neighborhood and home to the hottest, most massive stars known. This makes it a perfect natural laboratory in which to test out theories of star formation and evolution, and Hubble has a rich variety of images of this region. The NASA/ESA/CSA James Webb Space Telescope also recently delved into this region, revealing thousands of never-before-seen young stars.
This new image combines data from two different observing proposals. The first was designed to explore the properties of the dust grains that exist in the void between stars that make up the dark clouds winding through this image. This proposal, which astronomers named Scylla, reveals how interstellar dust interacts with starlight in a variety of environments. It complements another Hubble program called Ulysses, which characterizes the stars. This image also incorporates data from an observing program studying star formation in conditions similar to the early universe, as well as cataloging the stars of the Tarantula Nebula for future science with Webb.
Text credit: European Space Agency (ESA)
Image credit: ESA/Hubble & NASA, C. Murray, E. Sabbi; Acknowledgment: Y. -H. Chu
For more information: www.nasa.gov/image-feature/goddard/2023/hubbles-new-view-...
The Universe is a dusty place, as this NASA/ESA Hubble Space Telescope Picture of the Week shows. Featured in this image are swirling clouds of gas and dust near the Tarantula Nebula in the Large Magellanic Cloud. About 160 000 light-years away in the constellations Dorado and Mensa, the Large Magellanic Cloud is one of the nearest galaxies to the Milky Way. The Tarantula Nebula is the most productive star-forming region in the nearby Universe, home to the most massive stars known.
The colourful gas clouds of this nebula are crossed by wispy tendrils and dark clumps of dust. This dust is different from ordinary household dust, which can be made of bits of soil, skin cells, hair and even plastic. Cosmic dust tends to be made of carbon or of molecules called silicates, which contain silicon and oxygen. The data used to create this image were collected as part of an observing programme that aims to characterise the properties of cosmic dust in the Large Magellanic Cloud and other nearby galaxies.
Dust plays several important roles in the Universe. Even though individual dust grains are incredibly tiny, far smaller than the width of a single human hair, dust grains in discs around young stars clump together to form larger grains and eventually planets. Dust also helps cool clouds of gas so that they can condense into new stars. Dust even plays a role in making new molecules in interstellar space, providing a venue for individual atoms to find each other and bond together in the vastness of space.
[Image Description: A portion of a nebula, made of variously-coloured layers of dust clouds. One upper layer is dark reddish dust which is dense and obscures light, in places so dense that it appears black. A middle layer is pale clouds that are thick like curling wisps of smoke. They form a broad bow across the centre of the image. Many small, bright stars lie throughout the nebula, coloured blue, purple or red depending on depth.]
Credits: ESA/Hubble & NASA, C. Murray; CC BY 4.0
Today’s NASA/ESA Hubble Space Telescope Picture of the Week features a dusty yet sparkling scene from one of the Milky Way’s satellite galaxies, the Large Magellanic Cloud. The Large Magellanic Cloud is a dwarf galaxy situated about 160 000 light-years away in the constellations Dorado and Mensa.
Despite being only 10–20% as massive as the Milky Way galaxy, the Large Magellanic Cloud contains some of the most impressive star-forming regions in the nearby Universe. The scene pictured here is on the outskirts of the Tarantula Nebula, the largest and most productive star-forming region in the local Universe. At its center, the Tarantula Nebula hosts the most massive stars known, which weigh in at roughly 200 times the mass of the Sun.
The section of the nebula shown here features serene blue gas, brownish-orange dust patches and a sprinkling of multicoloured stars. The stars within and behind the dust clouds appear redder than those that are not obscured by dust. Dust absorbs and scatters blue light more than red light, allowing more of the red light to reach our telescopes and making the stars appear redder than they are. This image incorporates ultraviolet and infrared light as well as visible light. Using Hubble observations of dusty nebulae in the Large Magellanic Cloud and other galaxies, researchers will study these distant dust grains, helping to understand the role that cosmic dust plays in the formation of new stars and planets.
[Image Description: A section of a nebula, made up of layers of coloured clouds of gas, of varying thickness. In the background are bluish, translucent and wispy clouds; on top of these are stretches of redder and darker, clumpy dust, mostly along the bottom and right. In the bottom left corner are some dense bars of dust that block light and appear black. Small stars are scattered across the nebula.]
Credits: ESA/Hubble & NASA, C. Murray; CC BY 4.0
This scene of stellar creation, captured by the Hubble Space Telescope, sits near the outskirts of the famous Tarantula Nebula, the largest known stellar nursery in the local universe. Called LHA 120-N 150, this cloud of gas and dust, along with the many young and massive stars surrounding it, is the perfect laboratory to study the origin of massive stars. The nebula is situated more than 160,000 light-years away in the Large Magellanic Cloud, a neighboring dwarf irregular galaxy that orbits our galaxy, the Milky Way.
Also known as 30 Doradus or NGC 2070, the Tarantula Nebula owes its name to the arrangement of bright patches that somewhat resemble the legs of a tarantula. It measures nearly 1,000 light-years across. Its proximity, the favorable inclination of the Large Magellanic Cloud, and the absence of intervening dust make the Tarantula Nebula one of the best laboratories in which to study the formation of stars, in particular massive stars. This nebula has an exceptionally high concentration of massive stars, often referred to as super star clusters.
Astronomers have studied LHA 120-N 150 to learn more about the environment in which massive stars form. Theoretical models of the formation of massive stars suggest that they should form within clusters of stars; but observations indicate that up to ten percent of them also formed in isolation. The giant Tarantula Nebula with its numerous substructures is the perfect laboratory in which to resolve this puzzle as in it massive stars can be found both as members of clusters and in isolation.
With the help of Hubble, astronomers are trying to find out whether the isolated stars visible in the nebula truly formed alone or just moved away from their stellar siblings. However, such a study is not an easy task; young stars, before they are fully formed — especially massive ones — look very similar to dense clumps of dust.
LHA 120-N 150 contains several dozen of these objects. They are a mix of unclassified sources — some probably young stellar objects and others probably dust clumps. Only detailed analysis and observations will reveal their true nature, and that will help to finally solve the unanswered question of the origin of massive stars.
For more information, please visit:
www.spacetelescope.org/videos/heic2004a/
Image credit: ESA/Hubble, NASA, I. Stephens
Text credit: European Space Agency
In the most active starburst region in the local universe lies a cluster of brilliant, massive stars, known to astronomers as Hodge 301. Hodge 301, seen in the lower right hand corner of this image, lives inside the Tarantula Nebula in our galactic neighbor, the Large Magellanic Cloud. This star cluster is not the brightest, or youngest, or most populous star cluster in the Tarantula Nebula, that honor goes to the spectacular R136. In fact, Hodge 301 is almost 10 times older than the young cluster R136. But age has its advantages; many of the stars in Hodge 301 are so old that they have exploded as supernovae. These exploded stars are blasting material out into the surrounding region at speeds of almost 200 miles per second. This high speed ejecta are plowing into the surrounding Tarantula Nebula, shocking and compressing the gas into a multitude of sheets and filaments, seen in the upper left portion of the picture. Hodge 301 contains three red supergiants — stars that are close to the end of their evolution and are about to go supernova, exploding and sending more shocks into the Tarantula. Also present near the center of the image are small, dense gas globules and dust columns where new stars are being formed today, as part of the overall ongoing star formation throughout the Tarantula region.
Credit: NASA/Hubble Heritage Project (STScI, AURA)
Image Number: PR99-12
Release Date: April 1, 1999
Exposure Date: December 17, 1995
The star-forming region, 30 Doradus, is one of the largest located close to the Milky Way and is found in the neighboring galaxy Large Magellanic Cloud. About 2,400 massive stars in the center of 30 Doradus, also known as the Tarantula Nebula, are producing intense radiation and powerful winds as they blow off material. Multimillion-degree gas detected in X-rays by NASA's Chandra X-ray Observatory comes from shock fronts formed by these stellar winds and by supernova explosions.
Credit: X-ray: NASA/CXC/PSU/L.Townsley et al.; Infrared: NASA/JPL/PSU/L.Townsley et al.
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My version of the Tarantula Nebula. Made from Webb Telescope data (wavelengths 90 + 187&200 combined + 335&444 combined)
Image attribution: NASA / ESA / CSA / Brian Tomlinson
Website: www.bt-photography.co.uk
Instagram: www.instagram.com/bt_photo
This is a showpiece of the southern skies, the Large Magellanic Cloud, a member of the Local Group, and a satellite galaxy of our Milky Way, one rich in star forming nebulas and clusters. The LMC is cross between a dwarf irregular galaxy and a barred spiral. The nebulas along its bar and arms show as regions of magenta and cyan, from hydrogen and oxygen emission.
The bright cyan Tarantula Nebula, NGC 2070, is at left, with the NGC 2014/NGC 1935 area above it.
The field is 7.5 by 5º but still does not include all the parts of the LMC.
This is a stack of 15 x 4-minute exposures with the Sharpstar 61mm EDPH III refractor at f/4.4 and the filter-modified (by AstroGear.net) Canon R at ISO 800, on the Astro-Physics AP400 mount autoguided with the MGEN3 autoguider. No filter was employed in the light path.
Taken March 3, 2024 from the Mirrabook Cottage near Coonabarabran, NSW, Australia, on the first night of a successul two-week observing run down under.
Several million young stars vie for attention in this Hubble Space Telescope image of a raucous stellar breeding ground in 30 Doradus, located in the heart of the Tarantula Nebula. Early astronomers nicknamed the nebula because its glowing filaments resemble spider legs.
30 Doradus is the brightest star-forming region visible in a neighboring galaxy and home to the most massive stars ever seen. Collectively, the stars in this image are millions of times more massive than our Sun. The image is roughly 650 light-years across and contains some rambunctious stars, from one of the fastest rotating stars to the speediest and most massive runaway star.
The image reveals the stages of star birth, from embryonic stars a few thousand years old still wrapped in cocoons of dark gas to behemoths that die young in supernova explosions. 30 Doradus is a star-forming factory, churning out stars at a furious pace over millions of years. Hubble shows star clusters of various ages, from about 2 million to about 25 million years old.
The region's sparkling centerpiece is a giant, young star cluster (left of center) named NGC 2070, only 2 million years old. Its stellar inhabitants number roughly 500,000. Its dense core, known as R136, is packed with some of the heftiest stars found in the nearby universe, weighing more than 100 times the mass of our Sun.
The massive stars are carving deep cavities in the surrounding material by unleashing a torrent of ultraviolet light, which is etching away the enveloping hydrogen gas cloud in which the stars were born. When the radiation hits dense walls of gas, it creates shocks, which may be generating a new wave of star birth.
The composite image comprises one of the largest mosaics ever assembled from Hubble photos and includes observations taken by Hubble's Wide Field Camera 3 and Advanced Camera for Surveys. The Hubble image is combined with ground-based data of the Tarantula Nebula, taken with the European Southern Observatory's 2.2-meter telescope in La Silla, Chile. NASA and the Space Telescope Science Institute released the image to celebrate Hubble's 22nd anniversary.
For more information, visit:
hubblesite.org/contents/news-releases/2012/news-2012-01.html
Credit: NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)
The area is rich in Integrated Flux Nebulae. A part of Gum Nebula is visible red near the left upper corner. Stars trailed near the left lower corner due to differential atmospheric refraction near the horizon.
Integrated Flux Nebulae are visible clearer in inverted frame.
Large Magellanic Cloud and Integrated Flux Nebulae Nearby with Sigma 85mmF1.4 Art December 2016 Inverted Version:
www.flickr.com/photos/hiroc/37527361541
The Magellanic Clouds are connected with stellar streams, the brightest parts of which are known as wing and tail of SMC. The MCs are also accompanied by long Hydrogen-I gas stream extending more than 100 degrees.
equipment: Sigma 40mmF1.4 Art and EOS 6D-SP4, modified by Seo-san on ZWO AM5 equatorial mount on the genuine tripod with counter weight 4.8kg, autoguided with Fujinon 1:2.8/75mm C-Mount Lens, ZWO ASI 120MM-mini, and PHD2 Guiding
exposure: 3 times x 900 seconds, 3 x 240 sec, 5 x 60, and 1 x 15 seconds at ISO 1,600 and f/3.2
site: 2,434m above sea level at lat. 24 39 52 south and long. 70 16 11 west near Cerro Armazones in Sierra Vicuña Mackenna in Coast Range of Chile
Ambient temperature was around 10 degrees Celsius or 34 degrees Fahrenheit. Wind was mild. Sky was dark, and SQML reached 21.83 at the night.
Description: This composite of 30 Doradus, aka the Tarantula Nebula, contains data from Chandra (blue), Hubble (green), and Spitzer (red). Located in the Large Magellanic Cloud, the Tarantula Nebula is one of the largest star-forming regions close to the Milky Way. Chandra's X-rays detect gas that has been heated to millions of degrees by stellar winds and supernovas. This high-energy stellar activity creates shock fronts, which are similar to sonic booms. Hubble reveals the light from massive stars at various stages of star birth, while Spitzer shows where the relatively cooler gas and dust lie.
Creator: Chandra X-ray Observatory Center
Date Created: 4/17/2012
Repository: Smithsonian Astrophysical Observatory
Image ID: 30dor
Permanent URL: chandra.harvard.edu/photo/2012/30dor/
The Tarantula is situated 170,000 light-years away in the Large Magellanic Cloud (LMC) in the Southern sky and is clearly visible to the naked eye as a large milky patch. Astronomers believe that this smallish irregular galaxy is currently going through a violent period in its life. It is orbiting around the Milky Way and has had several close encounters with it. It is believed that the interaction with the Milky Way has caused an episode of energetic star formation - part of which is visible as the Tarantula Nebula. Just above the centre of the image there is a huge cluster of very hot stars called R136. The stars in R136 are also among the most massive stars we know. R136 is also a very young cluster, its oldest stars being "just" 5 million years old or so. Its smallest stars, however, are still forming, so astronomers observe R136 to try to understand the early stages of stellar evolution. Near the lower edge of the image we find the star cluster Hodge 301. Hodge 301 is almost 10 times older than R136. Some of the stars in Hodge 301 are so old that they have already exploded as supernovae. The shockwave from this explosion has compressed the gas in the Tarantula into the filaments and sheets that are seen around the cluster. This mosaic of the Tarantula Nebula consists of images from the NASA/ESA Hubble Space Telescope's Wide Field and Planetary Camera 2 (WFPC2) and was created by 23 year old amateur astronomer Danny LaCrue. The image was constructed by 15 individual exposures taken through three narrow-band filters allowing light from ionised oxygen (501 nm, shown as blue), hydrogen-alpha (656 nm, shown as green) and ionised sulphur (672 nm, shown as red). The exposure time for the individual WFPC2 images vary between 800 and 2800 seconds in each filter. The Hubble data have been superimposed onto images taken through matching narrow-band filters with the European Southern Observatory's New Technology Telescope at the La Silla Observatory, Chile. Additional image processing was done by the Hubble European Space Agency Information Centre.
The LMC is a nearby small galaxy, 160,000 light years away.
This negative image in black and white shows the Western half of the galaxy and its outskirts, including the huge bright Tarantula Nebula NGC 2070, near the centre.
The majority of objects in this image belong to the LMC, although some are foregroud stars in our own galaxy.
Imaging conducted on a field night with Macarthur Astronomical Society.
Object Details:
Large Magellanic Cloud.
PGC 17223
Constellation: Dorado and Mensa.
Distance: 160,000 light years.
Apparent size: 645.6′ x 549.5′
Actal size: 30,000 light years across.
Image:
Exposure: 64 x 30s, f/2.5, ISO800.
Date: 2019-01-04.
Location: The Oaks, NSW.
Conditions: Mostly clear.
Sky: semi-dark rural.
Moon: no
Processing: Deep Sky Stacker > GIMP.
Image dimensions: 15° x 10°
Cropping: no.
Gear:
Imaging camera: Canon EOS 60D, piggy-backed on telescope.
Lens 135mm Canon
Guiding: off.
Tracking: on.
Telescope mount: SkyWatcher EQ6-R.
Polar aligning: QHYCCD PoleMaster.
Editor's note: This is an archive image from 1999, part of our "Think Pink" gallery, in honor of Breast Cancer Awareness month: www.flickr.com/photos/28634332@N05/sets/72157625045060125/
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In the most active starburst region in the local universe lies a cluster of brilliant, massive stars, known to astronomers as Hodge 301. Hodge 301, seen in the lower right hand corner of this image, lives inside the Tarantula Nebula in our galactic neighbor, the Large Magellanic Cloud. This star cluster is not the brightest, or youngest, or most populous star cluster in the Tarantula Nebula, that honor goes to the spectacular R136. In fact, Hodge 301 is almost 10 times older than the young cluster R136. But age has its advantages; many of the stars in Hodge 301 are so old that they have exploded as supernovae. These exploded stars are blasting material out into the surrounding region at speeds of almost 200 miles per second. This high speed ejecta are plowing into the surrounding Tarantula Nebula, shocking and compressing the gas into a multitude of sheets and filaments, seen in the upper left portion of the picture. Hodge 301 contains three red supergiants -- stars that are close to the end of their evolution and are about to go supernova, exploding and sending more shocks into the Tarantula. Also present near the center of the image are small, dense gas globules and dust columns where new stars are being formed today, as part of the overall ongoing star formation throughout the Tarantula region.
Image credit: NASA, The Hubble Heritage Team, STScI, AURA
Original image:
grin.hq.nasa.gov/ABSTRACTS/GPN-2000-000946.html
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Dramatic stellar crib
One square degree image of the Tarantula Nebula and its surroundings. The spidery nebula is seen in the upper-centre of the image. Slightly to the lower-right, a web of filaments harbours the famous supernova SN 1987A. Many other reddish nebulae are visible in the image, as well as a cluster of young stars on the left, known as NGC 2100. Technical information: the image is based on observations carried out by Joao Alves (Calar Alto, Spain), Benoit Vandame and Yuri Beletsky (ESO) with the Wide Field Imager (WFI) at the 2.2-m telescope on La Silla.
Credit: ESO / R. Fosbury (ST-ECF)
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Astronomers created this infrared mosaic of the Tarantula Nebula (Caldwell 103) using exposures from Hubble’s Advanced Camera for Surveys and its Wide Field Camera 3 taken between 2011 and 2013.
Credit: NASA, ESA, and E. Sabbi (STScI)
For Hubble's Caldwell catalog website and information on how to find these objects in the night sky, visit:
A 4-panel mosaic of the Large Magellanic Cloud, a satellite galaxy of the Milky Way and visible only from the southern hemisphere. The field takes in most of the LMC and its numerous nebulas and clusters. Notable is the Tarantula Nebula, NGC 2070, the cyan-tinted nebula at far left, surrounded by many other NGC nebulas and clusters. At upper right is the second largest and brightest nebula complex in the LMC, NGC 1763, dubbed the LMC Lagoon, or the Bean Nebula.
This is a 4-panel mosaic taken March 31, 2016 from the Tibuc Cottage, Coonabarabran, NSW, Australia. Each panel is a stack of 4 x 3 minute exposures with the Borg 77mm f/4 astrographic refractor and filter-modified Canon 5D MkII at ISO 1600. Stitched in Photoshop.
This Hubble image, taken with the Wide Field and Planetary Camera 2, shows both the spindly, spidery filaments of gas that inspired the Tarantula Nebula’s name, as well as the intriguing structure of “bubbles” forming the so-called Honeycomb Nebula (lower left).
Credit: ESA/Hubble & NASA; Acknowledgments: Judy Schmidt (Geckzilla)
For Hubble's Caldwell catalog website and information on how to find these objects in the night sky, visit:
In the most active starburst region in the local universe lies a cluster of brilliant, massive stars, known to astronomers as Hodge 301, seen at the lower right of this Hubble image. Many of the stars in Hodge 301 are so old that they have exploded as supernovae, blasting material outward at speeds of almost 200 miles per second. This high-speed material plows into the surrounding Tarantula Nebula, shocking and compressing the gas into a multitude of sheets and filaments, seen in the upper left portion of the picture.
Credit: The Hubble Heritage Team (AURA/STScI/NASA)
For Hubble's Caldwell catalog website and information on how to find these objects in the night sky, visit:
Edited European Southern Observatory image of the Tarantula Nebula in the Large Magellanic Cloud. Color/processing variant.
Original caption: Glowing brightly about 160 000 light-years away, the Tarantula Nebula is the most spectacular feature of the Large Magellanic Cloud, a satellite galaxy to our Milky Way. This image from VLT Survey Telescope at ESO’s Paranal Observatory in Chile shows the region and its rich surroundings in great detail. It reveals a cosmic landscape of star clusters, glowing gas clouds and the scattered remains of supernova explosions.
This new Hubble image shows a cosmic creepy-crawly known as the Tarantula Nebula in infrared light. This region is full of star clusters, glowing gas, and thick dark dust. Created using observations taken as part of the Hubble Tarantula Treasury Project (HTTP), this image was snapped using Hubble's Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS). The Hubble Tarantula Treasury Project (HTTP) is scanning and imaging many of the many millions of stars within the Tarantula, mapping out the locations and properties of the nebula's stellar inhabitants. These observations will help astronomers to piece together an understanding of the nebula's skeleton, viewing its starry structure.
More information: www.spacetelescope.org/images/heic1402a/
Credit:
NASA, ESA, E. Sabbi (STScI)
The area is rich in Integrated Flux Nebulae. A part of Gum Nebula is visible red near the left upper corner. Stars trailed near the left lower corner due to differential atmospheric refraction near the horizon.
Integrated Flux Nebulae are visible clearer in inverted frame.
Large Magellanic Cloud and Integrated Flux Nebulae Nearby with Sigma 85mmF1.4 Art December 2016 Inverted Version:
www.flickr.com/photos/hiroc/37527361541
The Magellanic Clouds are connected with stellar streams, the brightest parts of which are known as wing and tail of SMC. The MCs are also accompanied by long Hydrogen-I gas stream extending more than 100 degrees.
equipment: Sigma 40mmF1.4 Art and EOS 6D-SP4, modified by Seo-san on ZWO AM5 equatorial mount on the genuine tripod with counter weight 4.8kg, autoguided with Fujinon 1:2.8/75mm C-Mount Lens, ZWO ASI 120MM-mini, and PHD2 Guiding
exposure: 3 times x 900 seconds, 3 x 240 sec, 5 x 60, and 1 x 15 seconds at ISO 1,600 and f/3.2
site: 2,434m above sea level at lat. 24 39 52 south and long. 70 16 11 west near Cerro Armazones in Sierra Vicuña Mackenna in Coast Range of Chile
Ambient temperature was around 10 degrees Celsius or 34 degrees Fahrenheit. Wind was mild. Sky was dark, and SQML reached 21.83 at the night.
This is a frame of old data, left unprocessed.
Tarantula Nebula is in Large Magellanic Cloud, and the distance is about 50kpc or 160kly. It is bright, about mag.8. If it were at the distance as Great Orion Nebula, about 412pc, Tarantula Nebula would have been brighter than now by 150k times, around mag. -7, far brighter than the brightest Venus or the same as 4-day moon.
equipment: Takahashi FSQ-106ED, F3 Reducer 0.6x, and EOS R6-SP5, modified by Seo-san on ZWO AM5 equatorial mount on the genuine tripod with counter weight 4.8kg, autoguided with Fujinon 1:2.8/75mm C-Mount Lens, ZWO ASI 120MM-mini, and PHD2 Guiding
exposure: 4 times x 900 seconds, 3 x 240 sec, 5 x 60 sec, 3 x 15 sec, and 4 x 4 seconds at ISO 1,600 and f/3.0
site: 2,434m above sea level at lat. 24 39 52 south and long. 70 16 11 west near Cerro Armazones in Sierra Vicuña Mackenna in Coast Range of Chile
Ambient temperature was around 10 degrees Celsius or 34 degrees Fahrenheit. Wind was mild. Sky was dark, and SQML reached 21.83 at the night.
The Large Magellanic Cloud Central.
Central Region of The Large Magellanic Cloud.
Mosaic Panels: 3
Exposures per mosaic panel: R:5 hours + Ha:5 hours , B:5 hours + OIII: 5 hours (20 hours per tile, 60 hours total)
Total Field Covered: 240 x 130 arcminutes.
Dates: 12th, 13th, 22nd and 23rd November, 2nd, 3rd, 12th and 13th December 2009.
Location: Gold Coast, Queensland.
Processing:
Sub-Image calibration and per-filter colour image sigma rejected addition with CCDStack.
Background correction using the PixInsight software's Dynamic Background Extraction Tool.
Green Synthesis, RGB combination, mosaic assembly, levels and Adobe RGB 1998 colourspace conversion with Adobe Photoshop CS4.
Notes:
This image was an experiment in dealing with light pollution from my site by blending Narrowband filters with RGB and synthesizing Green, usually the most problematic colour.
Using Ha and OIII filters to limit the earthly glows and blending the flat backgrounds from these with standard Red and Blue filters.
For this particular image, being a mosaic, there is approximately 60 hours of exposures here without taking any Green or SII, which would have required another 30 hours of exposures in this case.
In an attempt to limit light pollution influences and also reduce the total amount of time needed to take all the exposures for this three-panel, pseudo RGB image, the Green channel was synthesised from the combined R = R+Ha and B= B+OIII images.
Telescope: Takahashi FSQ106ED
Focal Length: 390mm
Camera: SBIG ST10XE
Pixels: 2184 x 1472 x 6.7um
2010 Royal Observatory Greenwich -Astronomy Photographer of the Year shortlist.
The Large Magellanic Cloud (LMC), an irregular satellite galaxy of the Milky Way, and one of the prime attractions of the southern hemisphere sky. At left is the Tarantula Nebula, NGC 2070, while at upper right is the second brightest nebula in the LMC, NGC 1763, aka the LMC Lagoon. In between are an amazing number of nebulas, both magenta and cyan in tint, as well as clusters of stars. The LMC is 160,000 light years away, and is gravitationally bound to the Milky Way, though there is some dispute whether it is orbiting the Milky Way or is passing by.
This field is 6° x 4°, which just encompasses the majority of the LMC's structure and features.
I shot this Monday, March 24, 2014 from the Warrumbungles Mountain Motel grounds, near Coonabarabran, NSW, Australia. This is a stack of 6 x 10 minute exposures with the Borg 77mm aperture astrographic lens, a 300mm f/4 system, and the Canon 5D MkII camera, filter modified by Hutech, at ISO 800. Shots had to dodge clouds moving through during the evening. Humidity was high from rain earlier in the day. But transparency was good when skies were clear.
Description: The Chandra image of the Tarantula Nebula gives scientists a close-up view of the drama of star formation and evolution. The Tarantula, also known as 30 Doradus, is in one of the most active star-forming regions in a galaxy close to the Milky Way. Massive stars in 30 Doradus are producing intense radiation and searing winds of multimillion-degree gas that carve out gigantic super-bubbles in the surrounding gas. Other massive stars have raced through their evolution and exploded catastrophically as supernovas, leaving behind pulsars and expanding remnants that trigger the collapse of giant clouds of dust and gas to form new generations of stars.
Creator/Photographer: Chandra X-ray Observatory
The Chandra X-ray Observatory, which was launched and deployed by Space Shuttle Columbia on July 23, 1999, is the most sophisticated X-ray observatory built to date. The mirrors on Chandra are the largest, most precisely shaped and aligned, and smoothest mirrors ever constructed. Chandra is helping scientists better understand the hot, turbulent regions of space and answer fundamental questions about origin, evolution, and destiny of the Universe. The images Chandra makes are twenty-five times sharper than the best previous X-ray telescope. The Smithsonian Astrophysical Observatory controls Chandra science and flight operations from the Chandra X-ray Center in Cambridge, Massachusetts.
Medium: Chandra telescope x-ray
Date: 2008
Persistent URL: chandra.harvard.edu/photo/2008/30dor/
Repository: Smithsonian Astrophysical Observatory
Gift line: NASA/CXC/Penn State/L.Townsley
Accession number: 30dor
A 4-panel mosaic of the Large Magellanic Cloud, a satellite galaxy of the Milky Way and visible only from the southern hemisphere. The field takes in most of the LMC and its numerous nebulas and clusters. Notable is the Tarantula Nebula, NGC 2070, the cyan-tinted nebula at far left, surrounded by many other NGC nebulas and clusters. At right is the second largest and brightest nebula complex in the LMC, NGC 1763, dubbed the LMC Lagoon.
This is a 4-panel mosaic taken March 31, 2016 from the Tibuc Cottage, Coonabarabran, NSW, Australia. Each panel is a stack of 4 x 3 minute exposures with the Borg 77mm f/4 astrographic refractor and filter-modified Canon 5D MkII at ISO 1600. Stitched in Photoshop.
In the most active starburst region in the local universe lies a cluster of brilliant, massive stars, known to astronomers as Hodge 301.
Hodge 301, seen in the lower right corner of this image, lives inside the Tarantula Nebula within our galactic neighbor the Large Magellanic Cloud.
Many of the stars in Hodge 301 are so old that they have exploded as supernovae. These exploded stars are blasting material out into the surrounding region at speeds of almost 200 miles per second. This high-speed material is plowing into the surrounding Tarantula Nebula, shocking and compressing the gas into a multitude of sheets and filaments, seen in the upper left portion of the picture.
Hodge 301 contains three red supergiants — stars that are close to the end of their evolution and are about to go supernova, exploding and sending more shocks into the Tarantula.
Also present near the center of the image are small, dense gas globules and dust columns where new stars are being formed as part of the overall ongoing star formation throughout the Tarantula region.
For more information, visit: hubblesite.org/contents/news-releases/1999/news-1999-12.html
Credit: The Hubble Heritage Team (AURA/STScI/NASA)
The world in in complexe and in beauty
We live in it
Happy New Year 2013
Simone XXX
Please see it large and View On Black
the stars you see come from a a photo taken from Nasa Hubble it is 30 Doradus in Ultraviolet, Visible, and RED Light in the Tarantula Nebula
hubblesite.org/gallery/album/pr2009032c
The Dome you see is from inside the Oratoire Saint-Joseph in Montréal.
The Tarantula nebula in the LMC in Hubble palette narrowband colour (SII:Ha:OIII)
Taken with a SBIG STL6303E CCD camera on a 31.75cm Ritchey Chretien telescope working at F9.
200 minutes unbinned exposure with Astrodon 3nm Hydrogen Alpha filter with 240 minutes OIII and 260 minutes SII using 5nm Astrodon filters unbinned.
️ 30 Doradus - The Tarantula Nebula ️
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A cosmic masterpiece, the Tarantula Nebula (30 Doradus) lies within the Large Magellanic Cloud (LMC) and is one of the most dynamic star-forming regions in the Local Group of galaxies. Its spider-like web of glowing gas and young stars earned it the nickname Tarantula.
🔭 Target: 30 Doradus (Tarantula Nebula)
📍 Location: Constellation Dorado, approximately 160,000 light-years away
🌟 Apparent Magnitude: ~8
📐 Apparent Size: ~40 x 25 arcminutes
About the Region:
The Tarantula Nebula is a hotbed of stellar activity, housing some of the most massive and luminous stars known, such as those in the R136 cluster at its heart. This nebula is so luminous that, if it were as close as the Orion Nebula, it would cast shadows on Earth. The interplay of ultraviolet radiation and stellar winds sculpts intricate filaments of gas and dust, giving it its unique appearance.
🎨 Processing Notes:
The nebula's vibrant hues highlight emissions from hydrogen (Hα), oxygen (OIII), and sulfur (SII), revealing its intricate structure. This image emphasizes the nebula’s web-like formation and the dense star clusters embedded within.
Instrument: Telescope Takahashi FSQ-106ED, Camera FLI PL16803, Filters Astrodon Halpha, OIII, SII
Lights: Halpha 16x300", OIII 16x300", SII 16x300
#TarantulaNebula #30Doradus #LargeMagellanicCloud #Astrophotography #DeepSkyImaging
This composite image shows the star-forming region 30 Doradus, also known as the Tarantula Nebula. The background image, taken in the infrared, is itself a composite: it was captured by the HAWK-I instrument on ESO’s Very Large Telescope (VLT) and the Visible and Infrared Survey Telescope for Astronomy (VISTA), shows bright stars and light, pinkish clouds of hot gas. The bright red-yellow streaks that have been superimposed on the image come from radio observations taken by the Atacama Large Millimeter/submillimeter Array (ALMA), revealing regions of cold, dense gas which have the potential to collapse and form stars. The unique web-like structure of the gas clouds led astronomers to the nebula’s spidery nickname.
Credit: ESO, ALMA (ESO/NAOJ/NRAO)/Wong et al., ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit
©Xavier Fargas · All rights reserved
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... Foto-montaje del Faro de Santander
y pequeña Nube de Magallanes
... Photo-montage of Santander Lighthouse
and small Magellanic Cloud
PRIMER PLANO - FOREGROUND
Situado en el promontorio de Cabo Mayor, al norte de la ciudad de Santander, se ordenó construir un fanal giratorio por Real Orden del 17 de febrero de 1833. En este mismo lugar ya existía con anterioridad un atalayón desde el que se hacían señales a los barcos, tanto de día (con banderas) como de noche (con fuegos). El faro actual fue inaugurado seis años más tarde, el 15 de agosto de 1839.
FONDO - BACKGROUND
La Nebulosa de la Tarántula, también conocida como 30 Doradus o NGC 2070, es una región H II que se encuentra en la Gran Nube de Magallanes. Inicialmente considerada una estrella, en 1751 Nicolas Louis de Lacaille reconoció su naturaleza de nebulosa.
TARANTULA NEBULA
LRGB=3x10‘EACH, H-ALPHA,O-III, S-II=3x15‘ EACH
PLANEWAVE CDK 510 F6.8
FLI PL6303
REMOTE BY iTELESCOPE
SIDING SPRING, AUSTRALIA
S 31°16‘24“ E 149°03‘52“
Turning its 2.4-metre eye to the Tarantula Nebula, the NASA/ESA Hubble Space Telescope has taken this close-up of the outskirts of the main cloud of the Nebula.
The bright wispy structures are the signature of an environment rich in ionised hydrogen gas, called H II by astronomers. In reality these appear red, but the choice of filters and colours of this image, which includes exposures both in visible and infrared light, make the gas appear green.
More information: www.spacetelescope.org/images/potw1232a/
Credit:
ESA/Hubble & NASA
Acknowledgement: Judy Schmidt
Symphony of colours in the Tarantula
The Tarantula is situated 170,000 light-years away in the Large Magellanic Cloud (LMC) in the Southern sky and is clearly visible to the naked eye as a large milky patch. Astronomers believe that this smallish irregular galaxy is currently going through a violent period in its life. It is orbiting around the Milky Way and has had several close encounters with it. It is believed that the interaction with the Milky Way has caused an episode of energetic star formation – part of which is visible as the Tarantula Nebula.
Just above the centre of the image there is a huge cluster of very hot stars called R136. The stars in R136 are also among the most massive stars we know. R136 is also a very young cluster, its oldest stars being “just” 5 million years old or so. Its smallest stars, however, are still forming, so astronomers observe R136 to try to understand the early stages of stellar evolution. Near the lower edge of the image we find the star cluster Hodge 301. Hodge 301 is almost 10 times older than R136. Some of the stars in Hodge 301 are so old that they have already exploded as supernovae. The shockwave from this explosion has compressed the gas in the Tarantula into the filaments and sheets that are seen around the cluster.
This mosaic of the Tarantula Nebula consists of images from the NASA/ESA Hubble Space Telescope’s Wide Field and Planetary Camera 2 (WFPC2) and was created by 23 year old amateur astronomer Danny LaCrue. The image was constructed by 15 individual exposures taken through three narrow-band filters allowing light from ionised oxygen (501 nm, shown as blue), hydrogen-alpha (656 nm, shown as green) and ionised sulphur (672 nm, shown as red). The exposure time for the individual WFPC2 images vary between 800 and 2800 seconds in each filter. The Hubble data have been superimposed onto images taken through matching narrow-band filters with the European Southern Observatory’s New Technology Telescope at the La Silla Observatory, Chile. Additional image processing was done by the Hubble European Space Agency Information Centre.
Credit: ESA/NASA, ESO and Danny LaCrue
Edited European Southern Observatory image of the Tarantula Nebula (30 Doradus) in the Large Magellanic Cloud.
Original caption: This image of the dramatic star formation region 30 Doradus, also known as the Tarantula Nebula, was created from a mosaic of images taken using the HAWK-I instrument working with the Adaptive optics Facility of ESO’s Very Large Telescope in Chile. The stars are significantly sharper than the same image without adaptive optics being used, and fainter stars can be seen.