NGC 1035
| NGC 1035 | |
|---|---|
 Image of NGC 1035 obtained from the Sloan Digital Sky Survey | |
| Observation data | |
| Constellation | Cetus |
| Right ascension | 02h 40m 44s |
| Declination | -08° 01’ 28” |
| Absolute magnitude (B) | 12.89 |
| Surface brightness | 22.36 |
| magnitude (J) | 10.12 |
| magnitude (H) | 9.42 |
| magnitude (K) | 9.13 |
| Characteristics | |
| Type | Spiral galaxy |
NGC 1035 is a spiral galaxy located in the Constellation of Cetus. It is situated close to the celestial equator making it at least partially visable on both sides of the hemisphere during certain times of the year.[1]
The neighboring galaxy NGC 1052-DF4 shows signs of being tidally disrupted and is missing most of its dark matter. The cause for this missing dark matter is from this galaxy stripping the dark matter from NGC 1052-DF4 and is now stripping apart the galaxy itself. Only the central regions of NGC 1052-DF4 remains unaffected.[2]
Supernova
[edit]SN 1990E is a Type ll supernova that occurred in this galaxy.[3]
References
[edit]- ^ "NGC 1035 - Spiral Galaxy in Cetus | TheSkyLive". theskylive.com. Retrieved 2025-06-14.
- ^ [email protected]. "New Hubble Data Explains Missing Dark Matter". www.esahubble.org. Retrieved 2025-06-14.
- ^ Schmidt, Brian P.; Kirshner, Robert P.; Schild, Rudy; Leibundgut, Bruno; Jeffery, David; Willner, S. P.; Peletier, Reynier; Zabludoff, Ann I.; Phillips, Mark M.; Suntzeff, Nicholas B.; Hamuy, Mario; Wells, Lisa A.; Smith, R. Chris; Baldwin, Jack A.; Weller, W. G. (June 1993). "Photometric and Spectroscopic Observations of SN 1990E in NGC 1035 Observational Constraints for Models of Type II Supernovae". The Astronomical Journal. 105: 2236. doi:10.1086/116602. ISSN 0004-6256.