Colour rendering of Orion Nebula area

This is a composite of three 1-min exposures of the Orion Nebula through narrow band filters centred on the 2.166 micron Br-gamma atomic hydrogen line (here reproduced in blue colour), the 1.257 micron [FeII] line (green) and the 2.12 micron 1-0 S(1) molecular hydrogen line (red). The colour coding reflects the ionisation state of the gas. Br-gamma traces hydrogen gas that is ionised by the well known Trapezium and other hot, young, stars in the region ; the [FeII] emission is emitted by high velocity fragments ejected during the birth of new stars in the OMC1 molecular cloud. The hollow filaments seen in molecular hydrogen result from shock heating of the molecular gas in the wake of the outflowing matter. In this image, the scale is 0.29 arcsec/pixel ; the field is 5x5 arcmin with North at the top and East to the left ; the seeing was around 0.5 arcsec.

Oikeudet:

ESO/N. Devillard

Kuvasta

Tunnistus:eso9805a
Tyyppi:Havainto
Julkaisupäivä:29. tammikuuta 1998
Vastaavat julkaisut:eso9805
Koko:450 x 450 px

Kohteesta

Nimi:Orion Nebula
Tyyppi:Milky Way : Nebula : Type : Star Formation
Etäisyys:1400 valovuotta
Constellation:Orion
Kategoria:Nebulae

Kuvaformaatit

Suuri JPEG
72,6 KB
Kokoruudun JPEG
154,9 KB

Taustakuvat

1024x768
159,3 KB
1280x1024
218,1 KB
1600x1200
271,6 KB
1920x1200
288,5 KB
2048x1536
365,1 KB

Koordinaatit

Position (RA):5 35 14.19
Position (Dec):-5° 22' 9.15"
Field of view:4.92 x 4.92 arcminutes
Suuntaus:Pohjoinen on 0.1° vasen pystysuuntaan nähden

Värit ja suotimet

KaistaAallonpituusTeleskooppi
Infrapuna
Br-gamma
2.166 μmNew Technology Telescope
SOFI
Infrapuna
Feiii
1.257 μmNew Technology Telescope
SOFI
Infrapuna
H2
New Technology Telescope
SOFI