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Ss433_art_big.gif (717 × 469 piksel, ukuran berkas: 128 KB, tipe MIME: image/gif)

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Ringkasan

Deskripsi SS433 is one of the most exotic star systems known to astronomers. Its unremarkable name stems from its inclusion in a catalog of stars which emit radiation characteristic of atomic hydrogen. Its very remarkable behavior stems from a compact object, a black hole or neutron star, which has produced an accretion disk with jets. As illustrated in this artist's vision of the SS433 system based on observational data, a massive, hot star (left) is locked in a mutual orbit with a compact object. Material transfers from the massive star into an accretion disk surrounding the compact object blasting out two jets of ionized gas in opposite directions - at about 1/4 the speed of light! Radiation from the jet tilted toward the observer is blueshifted, while radiation from the jet tilted away is redshifted. The binary system itself completes an orbit in about 13 days while the jets precess (wobble like a top) with a period of about 164 days. Are the jets from SS433 related to those from black holes at the centers of galaxies?
Tanggal
Sumber https://apod.nasa.gov/apod/ap960306.html
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Public domain Berkas ini berada dalam domain publik di Amerika Serikat karena semata-mata diciptakan oleh NASA. Kebijakan hak cipta NASA menyatakan bahwa "materi NASA tidak dilindungi oleh hak cipta kecuali dicatat". (Lihat Template:PD-USGov, Halaman kebijakan hak cipta NASA atau JPL Image Use Policy.)
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Artist rendition of SS433, the first microquasar observed.

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terkini26 Oktober 2007 22.45Miniatur versi sejak 26 Oktober 2007 22.45717 × 469 (128 KB)Spacepotato{{Information |Description=Public domain work of NASA artist. Selected as Astronomy Picture Of The Day for March 6, 1996, <http://apod.nasa.gov/apod/ap960306.html>. |Source=<http://apod.nasa.gov/apod/image/ss433_art_big.gif>. |Date=unknown |Autho

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