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First black hole to have an accurate parallax measurement of its distance from our solar system B K [4] 0.7: Early K giant star 8100 ± 1000: 2.49 ± 0.30: GRO J0422+32: Binary star system with orbit t=5.09 h 04 h 21 m 42.723 s +32° 54′ 26.94″ 1992 Aug 5 A BH: 3.97 ± 0.95: B M1: 0.5 ± 0.1: 8150: 2.5: MACHO-96-BLG-5: Candidate isolated ...
OJ 287 core black holes — a BL Lac object with a candidate binary supermassive black hole core system [23] PG 1302-102 – the first binary-cored quasar — a pair of supermassive black holes at the core of this quasar [24] [25] SDSS J120136.02+300305.5 core black holes — a pair of supermassive black holes at the centre of this galaxy [26]
The Cosmic Background Explorer (COBE / ˈ k oʊ b i / KOH-bee), also referred to as Explorer 66, was a NASA satellite dedicated to cosmology, which operated from 1989 to 1993.Its goals were to investigate the cosmic microwave background radiation (CMB or CMBR) of the universe and provide measurements that would help shape our understanding of the cosmos.
A black hole with the mass of a car would have a diameter of about 10 −24 m and take a nanosecond to evaporate, during which time it would briefly have a luminosity of more than 200 times that of the Sun. Lower-mass black holes are expected to evaporate even faster; for example, a black hole of mass 1 TeV/c 2 would take less than 10 −88 ...
1 cm – edge of a cube of volume 1 mL; 1 cm – length of a coffee bean; 1 cm – approximate width of average fingernail; 1.2 cm – length of a bee; 1.2 cm – diameter of a die; 1.5 cm – length of a very large mosquito; 1.6 cm – length of a Jaragua Sphaero, a very small reptile; 1.7 cm – length of a Thorius arboreus, the smallest ...
97% chance of prompt collapse into a black hole immediately after merger. Alternative study suggests collapse 2.5 hours later. [4] [7] [8] [9] NGC 3201-1: 4.36 ± 0.41: 15,600 (see Notes) Spectroscopic radial velocity measurements of noninteracting companion. In globular cluster NGC 3201. Companion is 0.8M ☉ main sequence turn-off. [4] [10 ...
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