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Filaments in the Tarantula Nebula
Filaments of ionized gas in the proximity of the R136 cluster, which lies beyond the lower left edge of the photo. The different hues are due to different physical conditions that manifest themselves in the spectrum of the light emitted by the gas. Note also the dark lanes running roughly from bottom left to upper right, which are due to filaments of obscuring dust seen in projection against the background of bright nebulosity. The sky field measures 6.5 x 5.7 arcmin. North is up and East is left.
Kilde:ESO
Om billedet
Id: | eso0437b |
Type: | Observation |
Udgivelsesdato: | 10. december 2004 |
Relaterede pressemeddelelser: | eso0437 |
Størrelse: | 1628 x 1422 px |
Om objektet
Navn: | 30 Doradus, Tarantula Nebula |
Type: | Local Universe : Nebula : Appearance : Emission : H II Region Local Universe : Nebula : Type : Star Formation |
Afstand: | 170000 lysår |
Constellation: | Dorado |
Kategori: | Nebulae |
Baggrundsbilleder
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Koordinater
Position (RA): | 5 38 42.61 |
Position (Dec): | -69° 6' 3.89" |
Field of view: | 6.45 x 5.63 arcminutes |
Orientering: | Nord er 1.0° droite fra lodret |
Farver & filtre
Bånd | Teleskop |
---|---|
Ultraviolet U | Very Large Telescope WFI |
Optisk Oiii | Very Large Telescope WFI |
Optisk H-alpha | Very Large Telescope WFI |