NGC 1491
 | This article relies largely or entirely on a single source. (February 2017) |
| Emission nebula | |
|---|---|
 The nebula NGC 1491 | |
| Observation data: J2000 epoch | |
| Subtype | H II region |
| Right ascension | 04h 03m 15.9s[1] |
| Declination | +51° 18′ 54″[1] |
| Distance | 3.02 ± 0.6 kpc (9,800 ± 2,000 ly)[1] ly |
| Apparent dimensions (V) | ~1½° [2] |
| Constellation | Perseus |
| Designations | Ced 25, LBN 704, LBN 706, Sharpless 2-206[1], Little Pacman Nebula [3] |
NGC 1491, also known as LBN 704, SH2-206 or the Fossil Footprint Nebula, is an emission type bright nebula located about 9,800 light years away from Earth in the constellation of Perseus.[1] It was discovered on 23 December 1790 by William Herschel.
The nebula gets its deep red coloration due to many massive stars (such as BD+50 866) embedded within NGC 1491 producing large amounts of ultraviolet radiation and ionizing the hydrogen gas that makes up the nebula.[4][5]
Gallery
[edit]-
NGC 1491 from the Mount Lemmon Sky Center -
Closeup of NGC 1491 - Peter Kennett
References
[edit]- ^ a b c d e "NGC 1491". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 February 2017.
- ^ https://www.webbdeepsky.com/picture-of-the-month/archive/2024
- ^ https://www.deepskycorner.ch/obj/ngc1491.en.php
- ^ "Emission Nebula NGC 1491". noirlab.edu. Retrieved 2023-11-26.
- ^ "NGC 1491". Stargazers Lounge. 2021-03-08. Retrieved 2023-11-26.
External links
[edit]
Media related to NGC 1491 at Wikimedia Commons
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