NGC281
Star-forming region · Emission nebula in the constellation Cassiopeia
About NGC281
NGC281 is about 9,188 light-years from the Sun, so the light we see from it left about 9,188 years ago.
It is 32,895 light-years from the centre of the Milky Way.
The map lists it as a star-forming region (star-forming region (maser)) and shows it among the stars around the Sun, drawn on the plane of the Milky Way.
A water or methanol maser in a massive star-forming region. Radio telescopes measured its parallax directly, which is how the Milky Way's spiral arms are mapped.
Key numbers
| Distance | 9,188 light-years (2,817 pc) |
|---|---|
| Distance from the Galactic centre | 32,895 light-years |
| Galactic coordinates | l = 123.07°, b = -6.31° |
| Parallax | 0.355 mas (VLBI) |
| Spiral arm (Reid 2019) | Perseus Arm |
Data: Reid et al. 2019.
Where it is
Its place in the universe, from the inside out: Perseus Arm › Milky Way › Local Group › Virgo Supercluster › Laniakea Supercluster › Observable universe.
Zoom out to see it in context: Local Arm, a view about 12,000 light-years across.
From Wikipedia
NGC 281, IC 11 or Sh2-184 is a bright emission nebula and part of an H II region in the northern constellation of Cassiopeia and is part of the Milky Way's Perseus Spiral Arm. This 20×30 arcmin sized nebulosity is also associated with open cluster IC 1590, several Bok globules and the multiple star, B 1.
Excerpt from the Wikipedia article NGC 281, licensed CC BY-SA 4.0.
Nearby on the map
- Tycho's supernova remnant Supernova remnant
- NGC7538 Star-forming region
- Bubble Nebula Nebula
- Double Cluster Open star cluster
- Cassiopeia A Supernova remnant
- NGC 7789 Open star cluster