Wêne:M33.jpg
Mezinahiya vê pêşdîtinê: 600 × 600 pîksel. Resolusyonên din: 240 × 240 pîksel | 480 × 480 pîksel | 768 × 768 pîksel | 1024 × 1024 pîksel | 2048 × 2048 pîksel | 2904 × 2904 pîksel.
Dosyeya orjînal (2904 × 2904 pixel, mezinbûnê data: 775 KB, MIME-typ: image/jpeg)
|
Ev pel ji Wikimedia Commonsê ye. Agahdariya li ser rûpela danasîna pelê li jêr tê nîşandan. |
Danasîn
| Danasîn |
English: M33, the Triangulum Galaxy, is a perennial favorite of amateur and professional astronomers alike, due to its orientation and relative proximity to us. It is the second nearest spiral galaxy to our Milky Way (after M31, the Andromeda Galaxy) and a prominent member of the "local group" of galaxies. From our Milky Way perspective, M33's stellar disk appears at moderate inclination, allowing us to see its internal structure clearly, whereas M31 is oriented nearly edge-on.
The Galaxy Evolution Explorer imaged M33 as it appears in ultraviolet wavelengths. Ultraviolet imaging primarily traces emission from the atmospheres of hot stars, most of which formed in the past few hundred million years. These data provide a reference point as to the internal composition of a typical star-forming galaxy and will help scientists understand the origin of ultraviolet emission in more distant galaxies. These observations of M33 allow astronomers to compare the population of young, massive stars with other components of the galaxy, such as interstellar dust and gas, on the scale of individual giant molecular clouds. The clouds contain the raw material from which stars form. This presents direct insight into the star formation process as it occurs throughout an entire spiral galaxy and constitutes a unique resource for broader studies of galaxy evolution. |
| Dîrok | |
| Çavkanî | http://photojournal.jpl.nasa.gov/gallery/universe?subselect=Target:M33 |
| Xwedî | NASA/JPL-Caltech |
Lîsans
|
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
 |
Warnings:
|
Dîroka daneyê
Ji bo dîtina guhartoya wê demê bişkoka dîrokê bitikîne.
| Dîrok/Katjimêr | Wêneyê biçûk | Mezinahî | Bikarhêner | Şirove | |
|---|---|---|---|---|---|
| niha | 20:25, 11 çiriya paşîn 2005 | | 2904 x 2904 (775 KB) | Shaqspeare | |
| 15:55, 12 îlon 2005 |  | 162 x 162 (5 KB) | Emijrp | The spiral galaxy M33, Triangulum Galaxy. '''SOURCE:''' http://www.ipac.caltech.edu/2mass/gallery/messiercat.html <br> '''Acknowledgment:''' ''Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint proje |
Bikaranîna pelê
Ev rûpelên li jêr vê dosyeyê bi kar tînin:
Bikaranîna gerdûnî ya pelê
Ev wîkiyên di rêzê de vê pelê bi kar tînin:
- Bikaranîna di af.wikipedia.org de
- Bikaranîna di ar.wikipedia.org de
- Bikaranîna di ast.wikipedia.org de
- Bikaranîna di az.wikipedia.org de
- Bikaranîna di ba.wikipedia.org de
- Bikaranîna di be.wikipedia.org de
- Bikaranîna di bg.wikipedia.org de
- Bikaranîna di ca.wikipedia.org de
- Bikaranîna di ce.wikipedia.org de
- Bikaranîna di cs.wikipedia.org de
- Bikaranîna di cy.wikipedia.org de
- Bikaranîna di de.wikipedia.org de
- Bikaranîna di diq.wikipedia.org de
- Bikaranîna di el.wikipedia.org de
- Bikaranîna di en.wikipedia.org de
- Bikaranîna di en.wikibooks.org de
- Bikaranîna di eo.wikipedia.org de
- Bikaranîna di es.wikipedia.org de
- Bikaranîna di eu.wikipedia.org de
- Bikaranîna di fa.wikipedia.org de
- Bikaranîna di fr.wikipedia.org de
Zêdetir bikaranîna global a vê pelê bibîne.
