- H50 minutes (10 frames)
- S50 minutes (10 frames)
- O50 minutes (10 frames)
Sh2-103, also known as RCW 32, is a bright emission nebula in the constellation Aquila, located about 7,500 light-years from Earth. This cosmic object was discovered in 1953 by astronomers Reed and Caldwell and is known for its rich red and blue colors. The nebula glows due to gas and dust illuminated by young stars at its center.
Star formation
Sh2-103 is an active star forming region.
- Central cluster: young stars formed from the gas and dust surrounding the nebula.
- Ionization: the bright light from these stars illuminates the gas and dust, creating a stunning visual effect and turning the nebula into an astrophotographic object.
Interactions between galaxies
An interesting aspect of Sh2-103 is its location on the border between the Milky Way and the Large Magellanic Cloud. This unique position allows scientists to study:
- Interactions between galaxies.
- The influence of material ejected by the Large Magellanic Cloud on the formation of young stars in Sh2-103.
Scientific significance
Sh2-103 is a key object for studying star formation processes and the dynamics of galactic interactions. Its observations help astronomers understand:
- How gas and dust in nebulae turn into stars.
- How intergalactic matter affects the formation of star systems.
Bright and colorful, Sh2-103 continues to inspire both scientists and amateur astronomers with its breathtaking views and unique features.
Visibility chart of Nebula (Sh2-103) during the day
| Date | Moon Phase | Exposure | CCD Temperature | Gain | Offset | Filter |
|---|---|---|---|---|---|---|
- 2023ixf•
- 40 Eri•
- Abell 74•
- Artemis A868 SA•
- a Canis Minoris•
- C 2020 R4 ATLAS•
- C 2020 T2 Palomar•
- C 2021 S3 (PANSTARRS)•
- Haumea (2003 EL61)•
- HCG 68•
- HCG 92•
- IC 1318B•
- IC 1396•
- IC 1795•
- IC 1805•
- IC 1848•
- IC 1871•
- IC 3322A•
- IC 342•
- IC 4015•
- IC 405•
- IC 417•
- IC 434•
- IC 443•
- IC 4703•
- IC 5070•
- IC 5146•
- IC 63•
- M 1•
- M 101•
- M 103•
- M 109•
- M 13•
- M 15•
- M 27•
- M 3•
- M 33•
- M 42•
- M 45•
- M 5•
- M 51•
- M 57•
- M 63•
- M 64•
- M 74•
- M 76•
- M 81•
- M 82•
- M 86•
- M 87•
- M 94•
- M 97•
- NGC 147•
- NGC 1491•
- NGC 1499•
- NGC 1579•
- NGC 1961•
- NGC 2146•
- NGC 2239•
- NGC 2403•
- NGC 281•
- NGC 4236•
- NGC 4565•
- NGC 4631•
- NGC 507•
- NGC 508•
- NGC 5866•
- NGC 5907•
- NGC 6503•
- NGC 6823•
- NGC 6888•
- NGC 6946•
- NGC 6992•
- NGC 6995•
- NGC 7000•
- NGC 7023•
- NGC 7129•
- NGC 7217•
- NGC 7331•
- NGC 7380•
- NGC 7538•
- NGC 7635•
- NGC 7640•
- NGC 7822•
- NGC 891•
- NGC 896•
- NGC 925•
- PGC 54559•
- Sh2-155•
- Sh2-168•
- Sh2 103•
- Sh2 109•
- Sh2 132•
- T CrB•
- UGC 6930•
- V1405 Cas•
- Vesta A807 FA•