Although the Rosette nebula is not very bright - it is much too faint to see with the naked eye - it is famous mainly because it is a striking circular shape resembling a flower. The Rosette nebula is in the Perseus Arm of the Galaxy and has a young star cluster at the centre of it.
Four nebulae are listed in the NGC catalogue in the vicinity of the Rosette nebula although it is hard to determine precisely which parts of the Rosette Nebula they are meant to represent. They were all discovered visually in the eighteeth and nineteeth centuries before astronomers realised that there is only one nebula here. NGC 2239, for example seems to refer to a part of the nebula around the star 12 Monocerotis. The 'sizes' in this list refer to the entire nebula and not these individual parts.
1 2 3 4 5 6 7 8 Catalogue Equatorial Galactic Size Type Distance Size Other Names Number Coordinates Coordinates (arcmins) (ly) (ly) RA (2000) Dec l° b° -------------------------------------------------------------------------------------- NGC 2237 06 30.9 +05 03 206.1 -2.3 90' E 4700 125 Rosette nebula NGC 2238 06 30.7 +05 01 206.1 -2.3 90' E 4700 125 Rosette nebula NGC 2239 06 31.9 +04 57 206.3 -2.1 90' E 4700 125 Rosette nebula NGC 2246 06 32.6 +05 08 206.2 -1.8 90' E 4700 125 Rosette nebula |
Column 1: The standard catalogue name for the nebula. Column 2: Right Ascension and Declination for epoch 2000. Column 3: Galactic Longitude (l) and Latitude (b). Column 4: Angular size of the nebula in arcminutes. Column 5: Nebula type: E = emission, R = reflection. Column 6: Approximate distance to the nebula. Column 7: Approximate size of the nebula in light years. Column 8: Alternative name of the nebula.
The only star cluster which is definitely associated with the Rosette nebula is NGC 2244 at the centre of the nebula. This cluster was discovered by William Herschel in 1784. NGC 2186 is also in this list because although it is 5 degrees (and 400 light years) from Rosette nebula it is at the same distance from us. NGC 2252 at the northwest of the nebula may also be part of the nebula, although it has an unknown distance.
1 2 3 4 5 6 7 Catalogue Equatorial Galactic Size Distance Age Other Names Name Coordinates Coordinates (arcmins) (ly) (million RA (2000) Dec l° b° years) ------------------------------------------------------------------------------- NGC 2186 06 12.2 +05 28 203.6 -6.2 5' 4700 55 NGC 2244 06 32.0 +04 57 206.3 -2.1 29' 4700 8 NGC 2252 06 34.8 +05 22 206.2 -1.3 18' ? ? |
Column 1: The standard catalogue name for the cluster. Column 2: Right Ascension and Declination for epoch 2000. Column 3: Galactic Longitude (l) and Latitude (b). Column 4: Angular size of the cluster in arcminutes. Column 5: Distance to the cluster. Column 6: Approximate age of the cluster in millions of years. Column 7: Alternative name of the cluster. References: Dias W, Alessi B, Moitinho A, Lépine J, (2002). New catalogue of optically visible open clusters and candidates. Astron and Astrophys, 389, 871.
Below is a map of the Rosette Nebula. The principal parts of this nebula are labelled and the locations of the two main star clusters are also marked. Note also that the Rosette Nebula lies at the right end of a much fainter emission nebula that extends across three degrees of the sky.
The distance to the Rosette nebula is well known because there is a star cluster at the centre of the Rosette nebula which makes determining the distance much easier. The Rosette nebula is 4700 light years away and lies in the near side of the Perseus Arm. |
NGC 2244At the centre of the Rosette nebula is the NGC 2244 cluster. This young, bright cluster is responsible for creating the hole at the centre of the nebula. The intense radiation from the stars has blasted away the gas around them. This picture has a diameter of about 40 light years. |
NGC 2244. Image size: 0.5°x0.5°. DSS image. |
Dust lanes in NGC 2237. Image size: 0.15°x0.10°. DSS image. |
Dust lanes in the Rosette NebulaThis close-up view of part of the Rosette nebula reveals large clumps of dust. This picture has a width of approximately 10 light years. |