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MACS J0416.1-2403 är en galaxhop 4,3 miljarder ljusår från jorden i stjärnbilden Eridanus. Den har bildats av två kolliderande galaxhopar.
, MACS J0416.1-2403 is a cluster of galaxies … MACS J0416.1-2403 is a cluster of galaxies at a redshift of z=0.397 with a mass 160 trillion times the mass of the Sun inside 200 kpc (650 kly). Its mass extends out to a radius of 950 kpc (3,100 kly) and was measured as 1.15 × 1015 solar masses. The system was discovered in images taken by the Hubble Space Telescope during the Massive Cluster Survey, MACS. This cluster causes gravitational lensing of distant galaxies producing multiple images. Based on the distribution of the multiple image copies, scientists have been able to deduce and map the distribution of dark matter. The images, released in 2014, were used in the Cluster Lensing And Supernova survey with Hubble (CLASH) to help scientists peer back in time at the early Universe and to discover the distribution of dark matter. discover the distribution of dark matter.
, MACS J0416.1-2403是一個紅移值 z=0.397 的星系團，位於波江座。200 kpc範圍內質量為太陽的160兆倍。如果它的半徑是50 kpc，總質量則是太陽的1.15 x 1015倍。該星系團由發現（Massive Cluster Survey, MACS）。該星系團可使位於它後方遠處的星系產生重力透鏡效應，使一個星系產生多個影像。
, MACS J0416.1-2403 è un ammasso di galassie … MACS J0416.1-2403 è un ammasso di galassie situato in direzione della costellazione di Eridano con redshift di z=0,396 equivalente ad una distanza di 4,29 miliardi di anni luce. La sua massa è pari a 160 trilioni di masse solari entro i 200 kpc, mentre ad un raggio di 950 kpc è stata misurata in 1,15 x 1015 masse solari. MACS J0416.1-2403 è stato scoperto nel corso del MAssive Cluster Survey (MACS). L'osservazione dell'ammasso ha prodotto, tramite il fenomeno della lente gravitazionale, immagini multiple di galassie remote. Lo studio dell'ammasso è stato effettuato anche con osservazioni dei telescopi Hubble in luce visibile e Chandra nei raggi X. In particolare è stata individuata una galassia remota, la M0416 8958, a redshift di ~ 10, la cui immagine risale alle prime epoche di vita dell'Universo, circa 400 milioni di anni dopo il Big Bang.irca 400 milioni di anni dopo il Big Bang.
, MACS J0416.1-2403 es un cúmulo de galaxias … MACS J0416.1-2403 es un cúmulo de galaxias con un corrimiento al rojo de z=0,397 (aproximadamente cuatro mil millones de años luz) con una masa de 160 billones de veces la masa del Sol dentro de 200 kpc (650 kly). Su masa en un radio de 950 kpc (3.100 kly) se midió como 1,15×1015 masas solares. El sistema fue descubierto durante la MAssive Cluster Survey, MACS. Este cúmulo provoca lentes gravitacionales de galaxias distantes que producen múltiples imágenes. En 2015, se anunció que el cúmulo de galaxias proyectaba gravitacionalmente la galaxia más distante (z=12). Basándose en la distribución de las múltiples copias de imágenes, los científicos han podido deducir y mapear la distribución de la materia oscura.ar la distribución de la materia oscura.
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Galaxy cluster MCS J0416.1–2403 imaged by the Hubble Space Telescope
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MACS J0416.1–2403
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MACS J0416.1-2403, MACS J0416-2403, MACS 0416.1-2403, MACS 0416-2403, 1RXS J041609.9-240358
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MACS J0416.1-2403是一個紅移值 z=0.397 的星系團，位於波江座。200 kpc範圍內質量為太陽的160兆倍。如果它的半徑是50 kpc，總質量則是太陽的1.15 x 1015倍。該星系團由發現（Massive Cluster Survey, MACS）。該星系團可使位於它後方遠處的星系產生重力透鏡效應，使一個星系產生多個影像。
, MACS J0416.1-2403 is a cluster of galaxies … MACS J0416.1-2403 is a cluster of galaxies at a redshift of z=0.397 with a mass 160 trillion times the mass of the Sun inside 200 kpc (650 kly). Its mass extends out to a radius of 950 kpc (3,100 kly) and was measured as 1.15 × 1015 solar masses. The system was discovered in images taken by the Hubble Space Telescope during the Massive Cluster Survey, MACS. This cluster causes gravitational lensing of distant galaxies producing multiple images. Based on the distribution of the multiple image copies, scientists have been able to deduce and map the distribution of dark matter. The images, released in 2014, were used in the Cluster Lensing And Supernova survey with Hubble (CLASH) to help scientists peer back in time at the early Universe and to discover the distribution of dark matter. discover the distribution of dark matter.
, MACS J0416.1-2403 es un cúmulo de galaxias … MACS J0416.1-2403 es un cúmulo de galaxias con un corrimiento al rojo de z=0,397 (aproximadamente cuatro mil millones de años luz) con una masa de 160 billones de veces la masa del Sol dentro de 200 kpc (650 kly). Su masa en un radio de 950 kpc (3.100 kly) se midió como 1,15×1015 masas solares. El sistema fue descubierto durante la MAssive Cluster Survey, MACS. Este cúmulo provoca lentes gravitacionales de galaxias distantes que producen múltiples imágenes. En 2015, se anunció que el cúmulo de galaxias proyectaba gravitacionalmente la galaxia más distante (z=12). Basándose en la distribución de las múltiples copias de imágenes, los científicos han podido deducir y mapear la distribución de la materia oscura.ar la distribución de la materia oscura.
, MACS J0416.1-2403 è un ammasso di galassie … MACS J0416.1-2403 è un ammasso di galassie situato in direzione della costellazione di Eridano con redshift di z=0,396 equivalente ad una distanza di 4,29 miliardi di anni luce. La sua massa è pari a 160 trilioni di masse solari entro i 200 kpc, mentre ad un raggio di 950 kpc è stata misurata in 1,15 x 1015 masse solari.tata misurata in 1,15 x 1015 masse solari.
, MACS J0416.1-2403 är en galaxhop 4,3 miljarder ljusår från jorden i stjärnbilden Eridanus. Den har bildats av två kolliderande galaxhopar.
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| rdfs:label |
MACS0416.1-2403
, MACS J0416.1-2403
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