?? This collage of images from the NASA/ESA Hubble Space Telescope and the NASA/ESA/CSA James Webb Space Telescope provides a detailed view into the Flame Nebula ??? a hotbed of star formation less than 1 million years old! Webb’s near-infrared sensitivity allowed astronomers to identify three low-mass objects. These are so small that their cores will never be able to fuse hydrogen like full-fledged stars. Read more about it here: https://ow.ly/KIST50VeMI8 #WebbSeesFarther ?? NASA, ESA, CSA, M. Meyer (University of Michigan), A. Pagan (STScI)
ESA Hubble and Webb Space Telescopes
研究服务
Official ESA account for the #Hubble Space Telescope and the James #Webb Space Telescope.
关于我们
Official ESA account for the #Hubble Space Telescope and the James #Webb Space Telescope. Find us on esahubble.org and esawebb.org
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https://esahubble.org/
ESA Hubble and Webb Space Telescopes的外部链接
- 所属行业
- 研究服务
- 规模
- 11-50 人
- 总部
- Baltimore
- 类型
- 非营利机构
地点
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主要
Space Telescope Science Institute
US,Baltimore
ESA Hubble and Webb Space Telescopes员工
动态
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We’re getting ready to celebrate the NASA/ESA Hubble Space Telescope’s 35th anniversary! ?? To mark this very special day, ESA/Hubble has released a 2025 calendar featuring some of Hubble’s most spectacular anniversary images, from star clusters to spiral galaxies ?? Read more: https://ow.ly/E1qV50VcAK0 ?? ESA/Hubble
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Our ESA/Hubble Picture of the Week features a spiral paired with a prominent star! ? ?? The galaxy and the star appear close – but the star is 7109 light-years away in the Milky Way galaxy while the galaxy, NGC 4900, is 45 million light-years away! ?? This image combines data from two instruments on the NASA/ESA Hubble Space Telescope: the Advanced Camera for Surveys and the older Wide Field and Planetary Camera 2. The data used here were taken more than 20 years apart for two different observing programmes! ?? Both programmes aimed to understand the death of massive stars. In one, researchers studied the sites of past supernovae. In the other, they laid the groundwork for studying future supernovae ?? Read more: https://ow.ly/Mz3950VcAl0 ?? ESA/Hubble & NASA , S. J. Smartt, C. Kilpatrick
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?? The NASA/ESA/CSA James Webb Space Telescope has snapped an actively forming star system! ?? Near-infrared light captured by Webb shows incredible detail and structure in Lynds 483 (L483). Two actively forming stars are responsible for the ejection of gas and dust gleaming in orange, blue, and purple in this representative colour image. ?? These central protostars ?? have been ejecting gas and dust over tens of thousands of years, spewing it out as fast jets and slower outflows. When more recent ejections hit older ones, the material can tangle together. ?? Over time, chemical reactions within these ejections and the surrounding cloud have produced a range of molecules, including carbon monoxide, methanol, and other organic compounds. Read more about it here: https://ow.ly/NahT50VbMlY #WebbSeesFarther ?? NASA, ESA, CSA, STScI
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This artwork depicts a possible scenario for the 148780 Altjira system in the solar system’s Kuiper Belt: a hierarchical triple formation in which two close companions are orbited by a third. Read more: https://ow.ly/uTZC50Va7ti Artist's impression: NASA, ESA, J. Olmsted (STScI)
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?? The NASA/ESA/CSA James Webb Space Telescope has shed light on a starless super-Jupiter! ?? SIMP 0136 is a rapidly rotating, free-floating object roughly 13 times the mass of Jupiter. As the brightest object of its kind in the northern sky, it has long been an ideal target for exo-meteorology ??? ?? Astronomers knew that it varies in brightness, with patchy cloud layers that rotate in and out of view ?? although they didn’t know whether there were other factors at play. ?? Webb’s #NIRSpec and #MIRI monitored a broad spectrum of infrared light emitted by SIMP 0136 over two full rotations, detecting variations in cloud layers, temperature, and carbon chemistry. ?? This showed that SIMP 0136’s variations in brightness were due to a complex combination of atmospheric factors – not by clouds alone! Read more about it here: https://ow.ly/ZeNr50V9hOH #WebbSeesFarther Artist's impression: NASA, ESA, CSA, Joseph Olmsted (STScI)
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A very special day is coming up for the NASA/ESA Hubble Space Telescope ?? 24 April marks 35 years since Hubble was sent into orbit! Now, Hubble is more active and productive than ever. To celebrate its anniversary, ESA/Hubble has released a commemorative 2025 calendar, ‘Highlights from 35 Years of Discovery’, which looks back over a selection of Hubble’s most incredible images. Read more: https://ow.ly/6KhB50V9bGC ?? ESA/Hubble
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The spiral galaxy NGC 2283 ?? is one 55 star-forming galaxies observed by the NASA/ESA/CSA James Webb Space Telescope for a programme aiming to reveal the relationship between stars, gas, and dust in these galaxies. All 55 galaxies are close enough for Webb to see individual star clusters and gas clouds. These can be seen in this image outlining NGC 2283’s spiral arms! #WebbSeesFarther ?? ESA/Webb, NASA & CSA, A. Leroy, N. Bartmann (ESA/Webb) ?? Stellardrone - Twilight
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Our ESA/Hubble Picture of the Week features a spiral of the water snake ???? ?? NGC 5042 resides about 48 million light-years from Earth in the constellation Hydra (the water snake). It was captured in six wavelength bands, from the ultraviolet to the infrared, creating this multi-coloured portrait. ?? The galaxy’s cream-coloured centre is packed with ancient stars and its spiral arms are patched with young blue stars. Perhaps its most striking feature, however, is the collection of pink clouds spread throughout its spiral arms… ?? These are H II regions, which get their distinctive colour from hydrogen atoms that have been ionised by ultraviolet light. Only hot, massive stars ?? produce enough high-energy light to create these regions! Read more: https://ow.ly/mLPX50V97Ng ?? ESA/Hubble & NASA, D. Thilker
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Do you recognise this photo of the glittering open cluster Westerlund 1? ? You can find it alongside all our other ESA/Webb Pictures of the Month here: https://ow.ly/YaSv50V7vEY #WebbSeesFarther ?? ESA/Webb, NASA & CSA, M. Zamani (ESA/Webb), M. G. Guarcello (INAF-OAPA) and the EWOCS team
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