Datoteka:Threads of blue IC 4870.jpg
Izvorna datoteka (3.711 × 2.134 piksela, veličina datoteke: 3,66 MB, MIME tip: image/jpeg)
Ova datoteka je s Wikimedia Commonsa. Opis s njene stranice opisa datoteke prikazan je ispod. Commons je skladište slobodnih medija i datoteka za sve projekte fondacije Wikimedia. Možete i Vi pomoći. |
Sažetak
OpisThreads of blue IC 4870.jpg |
English: A ripple of bright blue threads through this galaxy like a misshapen lake system. The foreground of this image is littered with nearby stars with their gleaming diffraction spikes. A keen eye can also spot a few other galaxies that, while masquerading as stars at first glance, reveal their true nature on closer inspection.
The central galaxy streaked with colour, IC 4870, was discovered by DeLisle Stewart in 1900 and is located approximately 28 million light-years away. It contains an active galactic nucleus, or AGN: an extremely luminous central region so alight with radiation that it can outshine the rest of the galaxy put together. AGNs emit radiation across the complete electromagnetic spectrum, from radio waves to gamma-rays, produced by the action of a central supermassive black hole that is devouring material getting too close to it. IC 4870 is also a Seyfert galaxy, a particular kind of AGN with characteristic emission lines. IC 4870 has been imaged by Hubble for several studies of nearby active galaxies. By using Hubble to explore the small-scale structures of AGN in nearby galaxies, astronomers can observe the traces of collisions and mergers, central galactic bars, nuclear starbursts, jets or outflows, and other interactions between a galactic nucleus and its surrounding environment. Images such as this can help astronomers understand more about the true nature of the galaxies we see throughout the cosmos. |
Datum | |
Izvor | http://www.spacetelescope.org/images/potw1823a/ |
Autor | ESA/Hubble & NASA |
Licenciranje
ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
Conditions:
Notes:
|
- Slobodni ste:
- da dijelite – da kopirate, distributirate i prenosite djelo
- da remiksate – da prilagodite djelo
- Pod sljedećim uslovima:
- pripisivanje – Morate pripisati odgovarajuće autorske zasluge, osigurati link ka licenci i naznačiti jesu li napravljene izmjene. To možete uraditi na bilo koji razumni način, ali ne tako da se sugerira da davalac licence odobrava Vas ili Vašu upotrebu njegovog djela.
Items portrayed in this file
prikazuje
4 juni 2018
Historija datoteke
Kliknite na datum/vrijeme da vidite verziju datoteke iz tog vremena.
Datum/vrijeme | Smanjeni pregled | Dimenzije | Korisnik | Komentar | |
---|---|---|---|---|---|
trenutno | 18:45, 4 juni 2018 | 3.711 × 2.134 (3,66 MB) | Jmencisom | User created page with UploadWizard |
Upotreba datoteke
Sljedeća stranica koristi ovu datoteku:
Globalna upotreba datoteke
Sljedeći wikiji koriste ovu datoteku:
Metapodaci
Ova datoteka sadržava dodatne podatke koje je vjerovatno dodala digitalna kamera ili skener u procesu snimanja, odnosno digitalizacije. Ako je datoteka mijenjana, podaci možda nisu u skladu sa stvarnim stanjem.
Naslov slike |
|
---|---|
Pripisivanje/Pružalac usluga | ESA/Hubble & NASA |
Izvor | ESA/Hubble |
Kratki naslov |
|
Uslovi upotrebe |
|
Datum i vrijeme generisanja podataka | 06:00, 4 juni 2018 |
Komentar JPEG datoteke | A ripple of bright blue threads through this galaxy like a misshapen lake system. The foreground of this image is littered with nearby stars with their gleaming diffraction spikes. A keen eye can also spot a few other galaxies that, while masquerading as stars at first glance, reveal their true nature on closer inspection. The central galaxy streaked with colour, IC 4870, was discovered by DeLisle Stewart in 1900 and is located approximately 40 million light-years away. It contains an active galactic nucleus, or AGN: an extremely luminous central region so alight with radiation that it can outshine the rest of the galaxy put together. AGNs emit radiation across the complete electromagnetic spectrum, from radio waves to gamma-rays, produced by the action of a central supermassive black hole that is devouring material getting too close to it. IC 4870 is also a Seyfert galaxy, a particular kind of AGN with characteristic emission lines. IC 4870 has been imaged by Hubble for several studies of nearby active galaxies. By using Hubble to explore the small-scale structures of AGN in nearby galaxies, astronomers can observe the traces of collisions and mergers, central galactic bars, nuclear starbursts, jets or outflows, and other interactions between a galactic nucleus and its surrounding environment. Images such as this can help astronomers understand more about the true nature of the galaxies we see throughout the cosmos. |
Ključne riječi | IC 4870 |
Podaci za kontakt |
Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
IIM verzija | 4 |