alb9202769
SN 1604, Kepler's Supernova, 2D Graphic
![Over 400 years ago, Johannes Kepler and many others witnessed the appearance of a new "star" in the sky. Today, this object is known as the Kepler supernova remnant. Previously, astronomers have deduced that the Kepler remnant comes from a so-called Type Ia supernova, which is the result of a thermonuclear explosion of a white dwarf. New data from Chandra suggest that this white dwarf exploded after pulling material from a companion red giant star, and not from the merger with another white dwarf. In this graphic a two dimensional simulation of the Kepler supernova has been projected into three dimensions and converted back into a 2D graphic, to compare with Chandra and Spitzer data. Yellow shows high density gas and blue shows low density gas. The simulation does a good job at reproducing the disk-like structure [see #1 above] seen in the data. This supports the author's interpretation that the disk-like structure formed when interaction occurred between the supernova and a wind left behind by the giant star companion to the exploded star. Release date March 18, 2013.](/photos/prev/YWY2MjU4MA/album_alb9202769.webp)
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Título: SN 1604, Kepler's Supernova, 2D Graphic
Descripción: Ver traducción automática
Over 400 years ago, Johannes Kepler and many others witnessed the appearance of a new "star" in the sky. Today, this object is known as the Kepler supernova remnant. Previously, astronomers have deduced that the Kepler remnant comes from a so-called Type Ia supernova, which is the result of a thermonuclear explosion of a white dwarf. New data from Chandra suggest that this white dwarf exploded after pulling material from a companion red giant star, and not from the merger with another white dwarf. In this graphic a two dimensional simulation of the Kepler supernova has been projected into three dimensions and converted back into a 2D graphic, to compare with Chandra and Spitzer data. Yellow shows high density gas and blue shows low density gas. The simulation does a good job at reproducing the disk-like structure [see #1 above] seen in the data. This supports the author's interpretation that the disk-like structure formed when interaction occurred between the supernova and a wind left behind by the giant star companion to the exploded star. Release date March 18, 2013.
Over 400 years ago, Johannes Kepler and many others witnessed the appearance of a new "star" in the sky. Today, this object is known as the Kepler supernova remnant. Previously, astronomers have deduced that the Kepler remnant comes from a so-called Type Ia supernova, which is the result of a thermonuclear explosion of a white dwarf. New data from Chandra suggest that this white dwarf exploded after pulling material from a companion red giant star, and not from the merger with another white dwarf. In this graphic a two dimensional simulation of the Kepler supernova has been projected into three dimensions and converted back into a 2D graphic, to compare with Chandra and Spitzer data. Yellow shows high density gas and blue shows low density gas. The simulation does a good job at reproducing the disk-like structure [see #1 above] seen in the data. This supports the author's interpretation that the disk-like structure formed when interaction occurred between the supernova and a wind left behind by the giant star companion to the exploded star. Release date March 18, 2013.
Crédito: Album / NASA/CXC/NCSU / Science Source
Autorizaciones: ? Cesión de modelo: No - ? Cesión de propiedad: No
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Tamaño imagen: 3600 × 3523 px | 36.3 MB
Tamaño impresión: 30.5 × 29.8 cm | 1417.3 × 1387.0 in (300 dpi)
Palabras clave: 1604 • 2013 • ADVANCED • ARTE • ASTRONOMIA • CELESTE • CELESTIAL • CIELO • CIENCIA • CUERPO • DETECCIÓN • DIAGRAMA • EMISION • ESPACIAL • ESPACIALES • ESPACIO • ESPECTRÓMETRO • ESTELAR • ESTRELLA • EXPLOSION • GRAFICO • ILUSTRACION • ILUSTRACIONES • IMAGENES • OBSERVATORIO • PLANETARIO • PLANETARIOS • PROFUNDA • RADIACION • RADIACIONES • RAYOS X • REMANENTE • S. XXI • SIGLO XXI • SIGLO • SUPERNOVA
