Name in the directory:NGC_891
Category:Galaxy
Right Ascension:2h 22m 22.61s
Declination:+42° 28′ 3.00″
Total Exposure:8 часов 40 минут
Number of Frames:54
Link to FITS files:Download
- R120 minutes (12 frames)
- G90 minutes (9 frames)
- L210 minutes (22 frames)
- B100 minutes (11 frames)
The spiral galaxy NGC 891 is a large spiral galaxy spanning about 100,000 light-years. It is located about 30 million light-years from Earth in the direction of the constellation Andromeda. From our perspective, the galaxy is seen almost edge-on, making its appearance particularly interesting.
Structure and Features
- NGC 891 has a thin galactic disk and a central bulge of stars, similar to the structure of our own Milky Way.
- The galaxy is divided into two parts by a band of dark dust that runs through its center.
Dust Filaments
- One of the distinctive features is the presence of dust filaments that stretch for hundreds of light-years above and below the central line of the galaxy.
- These dust structures were probably ejected from the galaxy's disk by supernova explosions or intense star formation processes.
Astronomical Significance
NGC 891 is an interesting object to study because its edge-on view allows astronomers to better understand the structure and dynamics of spiral galaxies. Its dust filaments also provide important clues about processes such as active star formation and dust ejections.
Visibility chart of Spiral Galaxy (NGC 891) during the day
The height diagram of Spiral Galaxy (NGC 891) above the horizon during the current day for the observatory observation point in Orenburg (51.7, 55.2). The chart shows when the object is above the horizon and at what maximum height in degrees it rises. The data is relevant for the observation date: Saturday, 26 April 2025.
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•