The sky behind the hole
Behind every black hole on BlackHoles.fyi is a sky of stars and the glow of the Milky Way, its light bent on the way to you.
Most of the site's pictures show the sky as it looks from Earth. The site also draws ten real black holes that astronomers have measured, and for two of them the sky is drawn as it would look from the hole.
Each part carries a label saying how real it is: worked out from the physics, following a model another team published, chosen for the picture, or partly worked out and partly chosen.
The stars and the Milky Way behind the hole
Partly worked out from the physics
The hole's gravity bends their light, as a lens does.
The bending is traced, and each bright star sits at its catalogued place with its measured colour. The Milky Way's glow is NASA's map of the sky from Earth, stretched for contrast, and the stars' brightness is chosen so you can see them. Nine of the real black holes draw the sky from where they are instead: five in our Galaxy (Cygnus X-1, Gaia BH1, Gaia BH3, V404 Cygni and GRS 1915+105) from Gaia's stars, Sgr A* from the star cluster round it and the dust of the Galaxy's centre, and three outside it (M87*, TON 618 and 3C 273) from their host galaxy's glow and its own stars, modelled from measurements (for TON 618, whose host has never been seen, from scaling alone).
- NASA Goddard Scientific Visualization Studio, Deep Star Maps 2020
- van Leeuwen 2007, Validation of the new Hipparcos reduction, A&A 474, 653
- Høg and others 2000, The Tycho-2 catalogue of the 2.5 million brightest stars, A&A 355, L27
- NASA HEASARC, the Hipparcos and Tycho-2 tables
- ESA 1997, The Hipparcos and Tycho Catalogues, volume 1
- Ballesteros 2012, New insights into black bodies, EPL 97, 34008
The sky as seen from a real black hole
Partly worked out from the physics
Some of the real black holes show the sky from where they are, not from Earth.
Seen from the hole, the Milky Way is not Earth's view. The stars come from Gaia, the European Space Agency's star-mapping satellite, moved to this hole's place. The glow between them is a model fitted to Earth's sky. Over it we lay the dark bands of dust that cross the Milky Way, as they look from Earth. Where Gaia cannot see, we use Earth's sky itself. A panel beside the hole's picture lists which parts are measured, modelled, chosen or borrowed. The four holes outside our Galaxy have no Gaia stars to move; for now their sky is dark, which the panel says, and the glow of their own galaxy is a later step.
- Gaia Collaboration, Vallenari and others 2023, Gaia Data Release 3: Summary of the content and survey properties, A&A 674, A1
- Bailer-Jones and others 2021, Estimating distances from parallaxes. V. Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3, AJ 161, 147
- Miller-Jones and others 2021, Cygnus X-1 contains a 21-solar-mass black hole: implications for massive star winds, Science 371, 1046
- Stirling and others 2001, A relativistic jet from Cygnus X-1 in the low/hard X-ray state, MNRAS 327, 1273
- El-Badry and others 2023, A Sun-like star orbiting a black hole, MNRAS 518, 1057
- Gaia Collaboration, Panuzzo and others 2024, Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry, A&A 686, L2
- Reid and others 2014, A parallax distance to the microquasar GRS 1915+105 and a revised estimate of its black hole mass, ApJ 796, 2
- Kormendy and others 2009, Structure and formation of elliptical and spheroidal galaxies, ApJS 182, 216
- Mei and others 2007, The ACS Virgo Cluster Survey XIII: SBF distance catalog and the three-dimensional structure of the Virgo Cluster, ApJ 655, 144
- Oldham and Auger 2016, Evidence for a massive, extended globular cluster system around M87, from the Next Generation Virgo Survey, MNRAS
- Tamura and others 2006, Wide-field photometry of the globular clusters of M87 with Subaru, Papers I and II, MNRAS 373, 588 and 601
- Bahcall and others 1997, Hubble Space Telescope images of a sample of 20 nearby luminous quasars, ApJ 479, 642
- Ren and others 2024, HST/STIS coronagraph images of 3C 273's host galaxy, A&A 683, L5
- Loveday and others 2012, Galaxy And Mass Assembly (GAMA): ugriz galaxy luminosity functions, MNRAS 420, 1239
- Yasuda and others 2001, Galaxy number counts from the Sloan Digital Sky Survey commissioning data, AJ 122, 1104
- Shen and others 2003, The size distribution of galaxies in the Sloan Digital Sky Survey, MNRAS 343, 978
- Driver and others 2016, Measurements of extragalactic background light from the far UV to the far IR from deep ground and space-based galaxy counts, ApJ 827, 108
- Kormendy and Ho 2013, Coevolution (or not) of supermassive black holes and host galaxies, ARA&A 51, 511
- Vijaykumar and others 2024, Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes, ApJ 972, 157
- Artale and others 2020, Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time, MNRAS 491, 3419
- Cao, Lu and Zhao 2018, Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources, MNRAS 474, 4997
- Mapelli and others 2018, the host galaxies of double compact objects merging in the local Universe, MNRAS 481, 5324
- Bell and de Jong 2001, Stellar mass-to-light ratios and the Tully-Fisher relation, ApJ 550, 212
- Kregel, van der Kruit and de Grijs 2002, Flattening and truncation of stellar discs in edge-on spiral galaxies, MNRAS 334, 646
- Perna and others 2018, Binary black hole mergers within the LIGO horizon: statistical properties and prospects for detecting electromagnetic counterparts, MNRAS 477, 4228
- Varma, Isi and Biscoveanu 2020, Extracting the Gravitational Recoil from Black Hole Merger Signals, PRL 124, 101104
- Peng and others 2006, Probing the coevolution of supermassive black holes and galaxies using gravitationally lensed quasar hosts, ApJ 649, 616
- van der Wel and others 2014, 3D-HST+CANDELS: the evolution of the galaxy size-mass distribution since z = 3, ApJ 788, 28
- Schödel and others 2014, The nuclear cluster of the Milky Way: total mass and luminosity (long version), A&A 566, A47
- Schödel and others 2018, The distribution of stars around the Milky Way's central black hole II: diffuse light from sub-giants and dwarfs, A&A 609, A27
- Gallego-Cano and others 2020, New constraints on the structure of the nuclear stellar cluster of the Milky Way from star counts and MIR imaging, A&A 634, A71
- Fritz and others 2016, The nuclear cluster of the Milky Way: total mass and luminosity, ApJ 821, 44
- Sormani and others 2022, Self-consistent modelling of the Milky Way's nuclear stellar disc, MNRAS 512, 1857
- Launhardt, Zylka and Mezger 2002, The nuclear bulge of the Galaxy III: large-scale physical characteristics of stars and interstellar matter, A&A 384, 112
- Gillessen and others 2017, An update on monitoring stellar orbits in the Galactic Center, ApJ 837, 30
- Habibi and others 2017, Twelve years of spectroscopic monitoring in the Galactic Center: the closest look at S-stars near the black hole, ApJ 847, 120
- Paumard and others 2006, The two young star disks in the central parsec of the Galaxy: properties, dynamics, and formation, ApJ 643, 1011
- Schödel and others 2010, Peering through the veil: near-infrared photometry and extinction for the Galactic nuclear star cluster, A&A 511, A18
- NASA Goddard Scientific Visualization Studio, Deep Star Maps 2020
- ESA 1997, The Hipparcos and Tycho Catalogues, volume 1