| Kieli | Käännökset |
|---|---|
| bulgaria | че́рна ду́пка, черна дупка |
| espanja | agujero negro, hoyo negro |
| esperanto | nigra truo |
| hollanti | zwart gat |
| italia | buco nero |
| japani | ブラックホール (burakkuhōru / burakku hōru / burakku-hōru) |
| kreikka | μαύρη τρύπα (mávri trýpa), μελανή οπή (melaní opí) |
| latina | gurges ater |
| latvia | melnais caurums |
| liettua | juodoji skylė |
| portugali | buraco negro |
| puola | czarna dziura |
| ranska | trou noir |
| ruotsi | svart hål |
| saksa | schwarzes Loch |
| suomi | musta aukko |
| tanska | sort hul |
| turkki | kara delik |
| tšekki | černá díra |
| unkari | fekete lyuk |
| venäjä | чёрная дыра́ (tšornaja dyrá), чёрная дыра (tšornaja dyra) |
| viro | must auk |
| Monikko | black holes |
(physics) A region of spacetime that exerts a gravitational pull strong enough that no matter or energy, not even light, can escape it.
An image of the core region of Messier 87, a supermassive black hole, processed from a sparse array of radio telescopes known as the EHT with colors indicating brightness temperature.
(physics) A region of spacetime that exerts a gravitational pull strong enough that no matter or energy, not even light, can escape it.
Simulated view of a Schwarzschild black hole in front of the Large Magellanic Cloud. Note the gravitational lensing effect, which produces two enlarged but highly distorted views of the Cloud. Across the top, the Milky Way disk appears distorted into an arc.
(physics) A region of spacetime that exerts a gravitational pull strong enough that no matter or energy, not even light, can escape it.
The first simulated image of a black hole, created by Jean-Pierre Luminet in 1978 and featuring the characteristic shadow, photon sphere, and lensed accretion disk. The disk is brighter on one side due to the Doppler beaming.