PGC 10922

Koordinat: Peta langit 02h 53m 35.851s, −83° 08′ 31.85″

PGC 10922
PGC 10922 diambil oleh Teleskop Luar Angkasa Hubble
Kredit: ESA/Hubble & NASA Acknowledgement: Judy Schmidt
Data pengamatan (J2000 epos)
Rasi bintangOctans
Asensio rekta 02j 53m 35.851d[1]
Deklinasi -83° 08′ 31.85″[1]
Pergeseran merah0.0161[1]
Kecepatan radial helio4788 km/s[1]
Jarak200 million ly
Magnitudo semu (B)13.74[1]
Ciri-ciri
JenisS0[1]
Ukuran semu (V)1.3 x 1.1 arcmin
Penamaan lain
ESO 3-13, IRAS 02575-8320, IRAS F02575-8320, PSCz Q02575-8320, 6dFGS gJ025335.9-830832, PGC 10922, 2MASX J02533585-8308318

PGC 10922 adalah sebuah galaksi lentikular yang terletak 200 juta tahun cahaya dari Bumi.[2]

Referensi

  1. ^ a b c d e f "Search Results for PGC 10922". Astronomical Database. SIMBAD. Diakses tanggal 13 September 2013.
  2. ^ "Dark, dusty shells". ESA/Hubble Picture of the Week. Diakses tanggal 13 September 2013.

Content Disclaimer

Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.

  1. The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
  2. There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
  3. It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
  4. Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
  5. Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.
Kembali kehalaman sebelumnya