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    The Herschel Space Observatory has shown that galaxies with the most powerful

    The Herschel Space Observatory has shown that galaxies with the most powerful, active, supermassive black holes at their cores produce fewer stars than galaxies with less active black holes.、クレジット:World History Archive/ニューズコム/共同通信イメージズ ※エディトリアル使用のみ。広告、プロモーション、商業目的での利用に関してはお問合せください。

    商品コード: 2019072404102

  • -
    This artist‘s conception illustrates

    This artist‘s conception illustrates one of the most primitive supermassive black holes known (central black dot) at the core of a young, star-rich galaxy.、クレジット:World History Archive/ニューズコム/共同通信イメージズ ※エディトリアル使用のみ。広告、プロモーション、商業目的での利用に関してはお問合せください。

    商品コード: 2019072404568

  • 2005年01月31日
    Composite image of galaxy cluster MS0735.

    Composite image of galaxy cluster MS0735.6+7421, located about 2.6 billion light-years away in the constellation Camelopardalis. image shows dozens of galaxies bound together by gravity. In Jan. 2005, astronomers reported that a supermassive black hole, lurking in the central bright galaxy, generated the most powerful outburst seen in the universe.、クレジット:World History Archive/ニューズコム/共同通信イメージズ ※エディトリアル使用のみ。広告、プロモーション、商業目的での利用に関してはお問合せください。

    商品コード: 2019091002593

  • 2020年04月23日
    Hubble Spots Spirals Within a Spiral NASA SPACE HUBBLE

    Galaxy NGC 2273, the subject of this NASA/ESA Hubble Space Telescope image, hosts an inner ring and two outer “pseudorings,“ having so many distinct rings is rare and makes NGC 2273 unusual. Rings are created when a galaxy‘s spiral arms appear to loop around to nearly close upon one another, combined with a trick of cosmic perspective. NGC 2273‘s two pseudorings are formed by two swirling sets of spiral arms coming together, and the inner ring by two arcing structures nearer to the galactic center, which seem to connect in a similar way. These rings are not the only unique feature of this galaxy. NGC 2273 is also a Seyfert galaxy, a galaxy with an extremely luminous core. The center of a galaxy such as this is powered by a supermassive black hole and can glow brightly enough to outshine an entire galaxy like the Milky Way. NASA/UPI Photo via Newscom、クレジット:NASA/UPI/ニューズコム/共同通信イメージズ

    商品コード: 2020042703639

  • 2020年08月25日
    Fermi‘s Motion Produces A Study In Spirograph

    August 25, 2020 - USA - This image compresses the Vela movie sequence into a single snapshot by merging pie-slice sections from eight individual frames. NASA‘s Fermi Gamma-ray Space Telescope orbits our planet every 95 minutes, building up increasingly deeper views of the universe with every circuit. Its wide-eyed Large Area Telescope (LAT) sweeps across the entire sky every three hours, capturing the highest-energy form of light gamma rays from sources across the universe. These range from supermassive black holes billions of light-years away to intriguing objects in our own galaxy, such as X-ray binaries, supernova remnants and pulsars. (Credit Image: © NASA/ZUMA Wire/、クレジット:©NASA/ZUMA Wire/共同通信イメージズ

    商品コード: 2020082801104

  • 2020年10月03日
    The Hubble Space Telescope Observes Spectacular Supernova Time-Lapse HUBBLE SPACE SUPERNOVA

    Pictured here, in an image released on October 1, 2020, is the captivating galaxy NGC 2525. Located nearly 70 million light-years from Earth, this galaxy is part of Puppis‘ constellation in the southern hemisphere. Together with the Carina and the Vela constellations, it makes up an image of the Argo from ancient greek mythology. Another kind of monster, a supermassive black hole, lurks at the center of NGC 2525. Nearly every galaxy contains a supermassive black hole, which can range in mass from hundreds of thousands to billions of times the mass of the Sun.  Hubble has captured a series of images of NGC2525 as part of one of its major investigations; measuring the expansion rate of the Universe, which can help answer fundamental questions about our Universe‘s very nature. ESA/Hubble has now published a unique time-lapse of this galaxy, and it‘s fading supernova. NASA/ESA/UPI Photo via Newscom、クレジット:NASA/ESA/UPI/ニューズコム/共同通信イメージズ

    商品コード: 2020100704937

  • 2021年02月25日
    Galaxy NGC 1068

    February 25, 2021 - Space - A 2003 composite Chandra X-ray (blue/green) and Hubble optical (red) image of NGC 1068 shows hot gas blowing away from a central supermassive black hole at speeds averaging about 1 million miles per hour. The elongated shape of the gas cloud is thought to be due to the funneling effect of a torus, or doughnut-shaped cloud, of cool gas and dust that surrounds the black hole. The X-rays are scattered and reflected X-rays that are probably coming from a hidden disk of hot gas formed as matter swirls very near the black hole. Regions of intense star formation in the inner spiral arms of the galaxy are highlighted by the optical emission. (Credit Image: © Chandra/NASA/ZUMA Wire/、クレジット:©Chandra/NASA/ZUMA Wire/共同通信イメージズ

    商品コード: 2021030106668

  • 2021年04月16日
    Almost Every Galaxy Has A Black Hole

    April 16, 2021, Space: Spectacular jets are powered by the gravitational energy of a supermassive black hole in the core of the elliptical galaxy Hercules A. The jets shoot through space for millions of trillions of miles. This image, taken by the Hubble Telescope, was originally released in November 2012. (Credit Image: © NASA/ZUMA Wire/、クレジット:©NASA/ZUMA Wire/共同通信イメージズ

    商品コード: 2021041801652

  • 2021年11月26日
    Black Hole Collision May Have Exploded With Light

    November 26, 2021 - California, USA - In a first, astronomers may have seen light from the merger of two black holes, providing opportunities to learn about these mysterious dark objects. This artist‘s concept shows a supermassive black hole surrounded by a disk of gas. Embedded in this disk are two smaller black holes that may have merged together to form a new black hole.Ê When two black holes spiral around each other and ultimately collide, they send out gravitational waves, ripples in space and time that can be detected with extremely sensitive instruments on Earth. Since black holes and black hole mergers are completely dark, these events are invisible to telescopes and other light-detecting instruments used by astronomers. However, theorists have come up with ideas about how a black hole merger could produce a light signal by causing nearby material to radiate. The merger was identified on May 21, 2019, by two gravitational wave detectors, in an event called GW190521g. (Credit Image: © Caltech/NASA/Z...

    商品コード: 2021113009309

  • 2021年12月09日
    Hubble Finds Smoldering Remnant In Blast From The Past

    December 9, 2021 - Space - This is a composite of view of X-rays and warm ionized gas near the galactic center. The graphic of a translucent, vertical white fan is added to show the suggested axis of a mini-jet from the supermassive black hole at the galaxy‘s heart. The orange colored features are of glowing hydrogen gas. One such feature, at the top tip of the jet is interpreted at a hydrogen cloud that has been hit by the outflowing jet. The jet scatters off the cloud into tendrils that flow northward. Farther down near the black hole are X-ray observations of superheated gas colored green and blue. These date are circumstantial evidence that the black hole occasionally accretes stars or gas clouds, and ejects some of the superheated material along its spin axis. (Credit Image: © NASA/ZUMA Press Wire Service/、クレジット:©NASA/ZUMA Press Wire Service/共同通信イメージズ

    商品コード: 2022011510624

  • 2022年05月12日
    Black Hole At The Centre Of Our Galaxy Imaged For The First Time

    May 12, 2022, Milky Way Galaxy: Radio astronomers have imaged the super massive black hole at the centre of the Milky Way. It is only the second-ever direct image of a black hole, after the same team unveiled a historic picture of a more distant black hole in 2019. The long-awaited results, presented today by the Event Horizon Telescope (EHT) collaboration, show an image reminiscent of the earlier one, with a ring of radiation surrounding a darker disk of precisely the size that was predicted from indirect observations and from Albert Einstein‘s theory of gravity. (Credit Image: © Event Horizon Telescope/ZUMA Press Wire)、クレジット:©Event Horizon Telescope/ZUMA Press Wire/共同通信イメージズ

    商品コード: 2022052010972

  • 2022年05月13日

    12日、初めて撮影に成功した銀河系中心にあるブラックホールの写真。世界の天文学者らが参加する国際研究グループが12日、世界各地で記者会見を同時に開催し、天の川銀河の中心に存在する超大質量ブラックホールの写真を初公開した。これにより、撮影された天体が間違いなくブラックホールであることが実証され、多くの銀河の中心に存在すると考えられている巨大ブラックホールの働きを理解するための貴重な手掛かりとなった。写真は、国際共同研究プロジェクト「イベント・ホライズン・テレスコープ(EHT)」が世界各地の電波望遠鏡を連携させて撮った。(上海=新華社配信)= 配信日: 2022(令和4)年5月13日、クレジット:新華社/共同通信イメージズ

    商品コード: 2022051315025

  • 2022年05月13日

    12日、オンラインで開かれた記者会見で研究成果を解説する専門家。世界の天文学者らが参加する国際研究グループが12日、世界各地で記者会見を同時に開催し、天の川銀河の中心に存在する超大質量ブラックホールの写真を初公開した。これにより、撮影された天体が間違いなくブラックホールであることが実証され、多くの銀河の中心に存在すると考えられている巨大ブラックホールの働きを理解するための貴重な手掛かりとなった。写真は、国際共同研究プロジェクト「イベント・ホライズン・テレスコープ(EHT)」が世界各地の電波望遠鏡を連携させて撮った。(上海=新華社記者/金立旺)= 配信日: 2022(令和4)年5月13日、クレジット:新華社/共同通信イメージズ

    商品コード: 2022051315064

  • 2022年05月13日

    (220513) -- SHANGHAI, May 13, 2022 (Xinhua) -- Photo unveiled on May 12, 2022 shows the first image of the supermassive black hole at the center of the Milky Way galaxy. Astronomers revealed the first image of the supermassive black hole at the center of the Milky Way galaxy on Thursday. The image was produced by a global research team called the Event Horizon Telescope (EHT), using observations from a worldwide network of radio telescopes. (Event Horizon Telescope (EHT) via Xinhua)= 配信日: 2022(令和4)年5月13日、クレジット:新華社/共同通信イメージズ

    商品コード: 2022051310262

  • 2022年05月13日

    (220513) -- SHANGHAI, May 13, 2022 (Xinhua) -- Astronomers introduce research achievements at an online press conference on May 12, 2022. Astronomers revealed the first image of the supermassive black hole at the center of the Milky Way galaxy on Thursday. The image was produced by a global research team called the Event Horizon Telescope (EHT), using observations from a worldwide network of radio telescopes. (Xinhua/Jin Liwang)= 配信日: 2022(令和4)年5月13日、クレジット:新華社/共同通信イメージズ

    商品コード: 2022051310249

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