Astronomy Picture of the Day
Discover the cosmos! Each day a different image or photograph of our
fascinating universe is featured, along with a brief explanation
written by a professional astronomer.
2020 August 31
SS 433: Binary Star Micro-Quasar
Animation Credit: DESY, Science Communication Lab
Explanation: SS 433 is one of the most exotic star systems known. Its
unremarkable name stems from its inclusion in a catalog of Milky Way
stars which emit radiation characteristic of atomic hydrogen. Its
remarkable behavior stems from a compact object, a black hole or
neutron star, which has produced an accretion disk with jets. Because
the disk and jets from SS 433 resemble those surrounding supermassive
black holes in the centers of distant galaxies, SS 433 is considered a
micro-quasar. As illustrated in the animated featured video based on
observational data, a massive, hot, normal star is locked in orbit with
the compact object. As the video starts, material is shown being
gravitationally ripped from the normal star and falling onto an
accretion disk. The central star also blasts out jets of ionized gas in
opposite directions - each at about 1/4 the speed of light. The video
then pans out to show a top view of the precessing jets producing an
expanding spiral. From even greater distances, the dissipating jets are
then visualized near the heart of supernova remnant W50. Two years ago,
SS 433 was unexpectedly found by the HAWC detector array in Mexico to
emit unusually high energy (TeV-range) gamma-rays. Surprises continue,
as a recent analysis of archival data taken by NASA's Fermi satellite
find a gamma-ray source -- separated from the central stars as shown --
that pulses in gamma-rays with a period of 162 days - the same as SS
433's jet precession period - for reasons yet unknown.
Teachers & Students: Ideas for utilizing APOD in the classroom.
Tomorrow's picture: salted asteroid
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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Phillip Newman Specific rights apply.
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