Daftar lubang hitam paling masif

Sebuah gambaran seniman mengenai lubang hitam supermasif menelan materi dari piringan akresi

Berikut ini adalah sebuah daftar dari lubang hitam paling masif yang sejauh ini ditemukan (dan kandidat-kandidatnya), yang diukur dalam satuan massa matahari (M☉), sekitar 2×1030 kg.

Daftar

Daftar lubang hitam tersupermasif
Nama Massa matahari
(Matahari = 1) 		Catatan
TON 618 6,6×1010[1] Perkiraan dari korelasi garis emisi kuasar Hβ.
Holmberg 15A (4,0±0,8)×1010[2] Mass specified obtained through orbit-based, axisymmetric Schwarzschild models. Earlier estimates range from ~310 billion M☉ down to 3 billion M☉, all relying on empirical scaling relations and are thus obtained from extrapolation and not from kinematical measurements.[3]
IC 1101 (4–10)×1010[4] Perkiraan dari properti galaksi induk; massa belum diukur secara langsung.
S5 0014+81 4×1010[5][6][7] Sebuah makalah 2010 mengusulkan bahwa sebuah corong mengkolimasi radiasi di sekitar sumbu jet, menciptakan ilusi optik dengan kecerahan sangat tinggi, dan dengan demikian kemungkinan terjadi sebuah overestimasi pada massa lubang hitam tersebut.[5]
SMSS J215728.21-360215.1 (3,4±0,6)×1010[8]
SDSS J102325.31+514251.0 (3,31±0,61)×1010[9] Perkiraan dari korelasi garis emisi quasar MgII.
H1821+643 3×1010[10] Gugus galaksi terdekat yang mempunyai sebuah kuasar dalam intinya.[10]
NGC 6166 3×1010[11]
APM 08279+5255 2,3×1010[12]
1,0+0,17
−0,13×1010[13]		 Based on velocity width of CO line from orbiting molecular gas,[12] and reverberation mapping using SiIV and CIV emission lines.[13]
NGC 4889 (2,1±1,6)×1010[14][15] Best fit: the estimate ranges from 6 billion to 37 billion M☉.[14][15]
Central black hole of Phoenix Cluster 2×1010[16] This black hole is continuously growing at the rate of ~60 M☉ per year.
SDSS J074521.78+734336.1 (1,95±0,05)×1010[9] Estimated from quasar MgII emission line correlation.
OJ 287 primary 1,8×1010[17] A smaller 100 million M☉ black hole orbits this one in a 12-year period (see OJ 287 secondary below). But this measurement is in question due to the limited number and precision of observed companion orbits.
NGC 1600 (1,7±0,15)×1010[18][19] Unprecedentedly massive in relation of its location: an elliptical galaxy host in a sparse environment.
SDSS J08019.69+373047.3 (1,51±0,31)×1010[9] Estimated from quasar MgII emission line correlation.
SDSS J115954.33+201921.1 (1,41±0,10)×1010[9] Estimated from quasar MgII emission line correlation.
SDSS J075303.34+423130.8 (1,38±0,03)×1010[9] Estimated from quasar Hβ emission line correlation.
SDSS J080430.56+542041.1 (1,35±0,22)×1010[9] Estimated from quasar MgII emission line correlation.
Abell 1201 BCG (1,3±0,6)×1010[20] Estimated from the strong gravitational lensing of a background galaxy behind the BCG.[20] Beware of ambiguity between the BH mass determination and the galaxy cluster's dark matter profile.[21]
SDSS J0100+2802 (1,24±0,19)×1010[22][23] Estimated from quasar MgII emission line correlation. This object grew early in cosmic history (redshift 6.30).
SDSS J081855.77+095848.0 (1,20±0,06)×1010[9] Estimated from quasar MgII emission line correlation.
NGC 1270 1,2×1010[24] Elliptical galaxy located in the Perseus Cluster. Also is a low-luminosity AGN (LLAGN).[25]
SDSS J082535.19+512706.3 (1,12±0,20)×1010[9] Estimated from quasar Hβ emission line
SDSS J013127.34-032100.1 (1,1±0,2)×1010[26] Estimated from accretion disk spectrum modelling.[26]
PSO J334.2028+01.4075 1×1010[27] There are actually two black holes, orbiting at each other in a close pair with a 542-day period. The largest one is quoted, while the smaller one's mass is not defined.[27]
Black hole of central elliptical galaxy of RX J1532.9+3021 1×1010[28]
QSO B2126-158 1×1010[5]
NGC 1281 1×1010[29] Compact elliptical galaxy in the Perseus Cluster. Mass estimates range from 10 billion M☉ down to <5 billion M☉.[30]
SDSS J015741.57-010629.6 (9,8±1,4)×109[9]
NGC 3842 9,7+3,0
−2,5×109[14][15] 		Brightest galaxy in the Leo Cluster
SDSS J230301.45-093930.7 (9,12±0,88)×109[9] Estimated from quasar MgII emission line correlation.
SDSS J075819.70+202300.9 (7,8±3,9)×109[9] Estimated from quasar Hβ emission line correlation.
CID-947 6,9+0,8
−1,2×109[31] 		Constitutes 10% of the total mass of its host galaxy. Estimated from quasar Hβ emission line correlation.
SDSS J080956.02+502000.9 (6,46±0,45)×109[9] Estimated from quasar Hβ emission line correlation.
SDSS J014214.75+002324.2 (6,31±1,16)×109[9] Estimated from quasar MgII emission line correlation.
Messier 87 "Powehi"[32] 7,22+0,34
−0,40×109[33]
6,3×109[34] 		Central galaxy of the Virgo Cluster; the first black hole directly imaged.
NGC 5419 7,2+2,7
−1,9×109[35]		 Estimated from the stellar velocity distribution. A secondary satellite SMBH may orbit around 70 parsecs.[35]
SDSS J025905.63+001121.9 (5,25±0,73)×109[9] Estimated from quasar Hβ emission line correlation.
SDSS J094202.04+042244.5 (5,13±0,71)×109[9] Estimated from quasar Hβ emission line correlation.
QSO B0746+254 5×109[5]
QSO B2149-306 5×109[5]
SDSS J090033.50+421547.0 (4,7±0,2)×109[9] Estimated from quasar MgII emission line correlation.
Messier 60 (4,5±1,0)×109[36]
SDSS J011521.20+152453.3 (4,1±2,4)×109[9] Estimated from quasar Hβ emission line correlation.
QSO B0222+185 4×109[5]
Hercules A (3C 348) 4×109 Notable for its million light-year long relativistic jet.
Abell 1836-BCG 3,61+0,41
−0,50×109[37]
SDSS J213023.61+122252.0 (3,5±0,2)×109[9] Estimated from quasar Hβ emission line correlation.
SDSS J173352.23+540030.4 (3,4±0,4)×109[9] Estimated from quasar MgII emission line correlation.
SDSS J025021.76-075749.9 (3,1±0,6)×109[9] Estimated from quasar MgII emission line correlation.
NGC 1271 3,0+1,0
−1,1×109[38]		 Compact elliptical or lenticular galaxy in the Perseus Cluster.[39]
SDSS J030341.04-002321.9 (3,0±0,4)×109[9] Estimated from quasar MgII emission line correlation.
QSO B0836+710 3×109[5]
SDSS J224956.08+000218.0 (2,63±1,21)×109[9] Estimated from quasar Hβ emission line correlation.
SDSS J030449.85-000813.4 (2,4±0,50)×109[9] Estimated from quasar Hβ emission line correlation.
SDSS J234625.66-001600.4 (2,24±0,15)×109[9] Estimated from quasar Hβ emission line correlation.
PKS 2128-123 2,02×109[40]
ULAS J1120+0641 2×109[41][42]
QSO 0537-286 2×109[5]
NGC 3115 2×109[43]
Q0906+6930 2×109[44] Most distant blazar, at z = 5.47
QSO B0805+614 1,5×109[5]
Messier 84 1,5×109[45]
J100758.264+211529.207 ("Pōniuāʻena") (1,5±0,2)×109[46] Second most-distant quasar known
PKS 2059+034 1,36×109[40]
Abell 3565-BCG 1,34+0,21
−0,19×109[37]
NGC 7768 1,3+0,5
−0,4×109[15]
NGC 1277 1,2×109[47] Once thought to harbor a black hole so large that it contradicted modern galaxy formation and evolutionary theories,[48] re-analysis of the data revised it downward to roughly a third of the original estimate.[49] and then one tenth.[47]
Black hole of central elliptical galaxy of MS 0735.6+7421 1×109[50][51][52] Produced a colossal AGN outburst after accreting 600 million M☉ worth of material. BH mass not explicitly stated; just a lower limit. Requires assumptions about the efficiencies of gas accretion and jet power.[50][51][52]
QSO B225155+2217 1×109[5]
QSO B1210+330 1×109[5]
NGC 6166 1×109[53] Central galaxy of Abell 2199; notable for its hundred thousand light year long relativistic jet.
Cygnus A 1×109[54] Brightest extrasolar radio source in the sky as seen at frequencies above 1 GHz
Sombrero Galaxy 1×109[55] Bolometrically most luminous galaxy in the local universe and also the nearest billion-solar-mass black hole to Earth.
Markarian 501 9×108–3,4×109[56] Brightest object in the sky in very high energy gamma rays.
PG 1426+015 (1,298±0,385)×109[57]
467.740.000[58]
3C 273 (8,86±1,87)×108[57]
550.000.000[58]		 Kuasar terterang di langit
ULAS J1342+0928 8×108[59] Kuasar paling jauh[59] − saat ini tercatat sebagai kuasar terjauh dengan z=7.54[59]
Messier 49 5,6×108[60]
NGC 1399 5×108[61] Central galaxy of the Fornax Cluster
PG 0804+761 (6,93±0,83)×108[57]
190.550.000[58]
PG 1617+175 (5,94±1,38)×108[57]
275.420.000[58]
PG 1700+518 7,81+1,82
−1,65×108[57]
60.260.000[58]
NGC 4261 4×108[62] Notable for its 88.000 light-year long relativistic jet.[63]
PG 1307+085 (4,4±1,23)×108[57]
281 840 000[58]
SAGE0536AGN (3,5±0,8)×108[64][65] Constitutes 1.4% of the mass of its host galaxy
NGC 1275 3,4×108[66][67] Central galaxy of the Perseus Cluster
3C 390.3 (2,87±0,64)×108[57]
338.840.000[58]
II Zwicky 136 (4,57±0,55)×108[57]
144.540.000[58]
PG 0052+251 (3,69±0,76)×108[57]
218.780.000[58]
Messier 59 2,7×108[68] Lubang hitam tersebut memiliki sebuah rotasi retrograd.[69]
PG 1411+442 (4,43±1,46)×108[57]
79.430.000[58]
Markarian 876 (2,79±1,29)×108[57]
240.000.000[58]
Galaksi Andromeda 2,3×108 Galaksi besar terdekat ke Bima Sakti
PG 0953+414 (2,76±0,59)×108[57]
182.000.000[58]
PG 0026+129 (3,93±0,96)×108[57]
53.700.000[58]
Fairall 9 (2,55±0,56)×108[57]
79.430.000[58]
Markarian 1095 (1,5±0,19)×108[57]
182.000.000[58]
Messier 105 1,4×108–2×108[70]
Markarian 509 (1,43±0,12)×108[57]
57.550.000[58]
Sekunder dari OJ 287 1×108[17] The smaller black hole orbiting OJ 287 primary (see above).
RX J124236.9-111935 1×108[71] Observed by the Chandra X-ray Observatory to be tidally disrupting a star.[71][72]
Messier 85 1×108[73]
NGC 5548 (6,71±0,26)×107[57]
123.000.000[58]
PG 1211+143 (1,46±0,44)×108[57]
40.740.000[58]
Messier 88 8×107[74]
Messier 81 (Galaksi Bode) 7×107[75]
Markarian 771 (7,32±3,52)×107[57]
7,586×107[58]
Messier 58 7×107[76]
PG 0844+349 (9,24±3,81)×107[57]
2,138×107[58]
Centaurus A 5,5×107[77] Also notable for its million light-year long relativistic jet.[78]
Markarian 79 (5,24±1,44)×107[57]
5,25×107[58]
Messier 96 48.000.000[79] Estimates can be as low as 1.5 million solar masses
Markarian 817 (4,94±0,77)×107[57]
4,365×107[58]
NGC 3227 (4,22±2,14)×107[57]
3,89×107[58]
NGC 4151 primary 4×107[80][81]
3C 120 5,55+3,14
−2,25×107[57]
2,29×107[58]
Markarian 279 (3,49±0,92)×107[57]
4,17×107[58]
NGC 3516 (4,27±1,46)×107[57]
2,3×107[58]
NGC 863 (4,75±0,74)×107[57]
1,77×107[58]
Messier 82 (Cigar Galaxy) 3×107[82] Prototype starburst galaxy.[83]
Messier 108 2,4×107[84]
M60-UCD1 2×107[85] Constitutes 15% of the mass of its host galaxy.
NGC 3783 (2,98±0,54)×107[57]
9.300.000[58]
Markarian 110 (2,51±0,61)×107[57]
5.620.000[58]
Markarian 335 (1,42±0,37)×107[57]
6.310.000[58]
NGC 4151 secondary 10.000.000[81]
NGC 7469 (12,2±1,4)×106[57]
6.460.000[58]
IC 4329 A 9,90+17,88
−11,88×106[57]
5.010.000[58]
NGC 4593 5,36+9,37
−6,95×106[57]
8.130.000[58]
Messier 61 5×106[86]
Messier 32 1,5×106–5×106[87] Sebuah galaksi satelit katai di Galaksi Andromeda.
Sagittarius A* 4,3×106[88] Lubang hitam di pusat Bima Sakti.

Lihat pula

Referensi

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