World Library  
Flag as Inappropriate
Email this Article

Leo I (dwarf galaxy)

Article Id: WHEBN0000969161
Reproduction Date:

Title: Leo I (dwarf galaxy)  
Author: World Heritage Encyclopedia
Language: English
Subject: Local Group, David Dunlap Observatory Catalogue, Canes Venatici I (dwarf galaxy), Satellite galaxies of the Milky Way, Leo I
Publisher: World Heritage Encyclopedia

Leo I (dwarf galaxy)

Leo I
Leo I appears as a faint patch to the right of the bright star, Regulus.
Observation data (J2000 epoch)
Constellation Leo
Right ascension 10h 08m 27.4s[1]
Declination +12° 18′ 27″[1]
Redshift 285 ± 2 km/s[1]
Distance 820 ± 70 kly (250 ± 20 kpc)[2][3]
Type E;dSph[1]
Apparent dimensions (V) 9′.8 × 7′.4[1]
Apparent magnitude (V) 11.2[1]
Notable features Milky Way satellite
Other designations
UGC 5470,[1] PGC 29488,[1] DDO 74,[1] A1006,[1] Harrington-Wilson #1,[1] Regulus Dwarf[1]

Leo I is a photographic plates of the National Geographic Society – Palomar Observatory Sky Survey, which were taken with the 48-inch Schmidt camera at Palomar Observatory.[4][5]


  • Visibility 1
  • Mass 2
  • Star formation 3
  • Globular clusters 4
  • Regulus 5
  • References 6
  • External links 7


The proximity of Regulus and the low surface brightness make it a real challenge to observe it. Medium-sized amateur telescopes (15 cm or more) and a dark sky appear to be required for a sighting. But some reports of April 2013 tell that one observer with an 11 cm mini Dobson and even a refractor as small as 7 cm f/10 has sighted Leo I under very dark sky conditions.[6]


The measurement of radial velocities of some bright red giants in Leo I have made possible to measure its mass. It was found to be at least (2.0 ± 1.0) × 107 M. The results are not conclusive, and do not exclude or confirm the existence of a large dark matter halo around the galaxy. However, it seems to be certain that the galaxy does not rotate.[5]

It has been suggested that Leo I is a tidal debris stream in the outer halo of the Milky Way. This hypothesis has not been confirmed, however.[5]

Star formation

Typical to a dwarf galaxy, the metallicity of Leo I is very low, only one percent that of the Sun. Gallart et al. (1999) deduce from Hubble Space Telescope observations that the galaxy experienced a major increase (accounting for 70% to 80% of its population) in its star formation rate between 6 Ga and 2 Ga (billion years ago). There is no significant evidence of any stars that are more than 10 Ga old. About 1 Ga ago, star formation in Leo I appears to have dropped suddenly to an almost negligible rate. Some low-level activity may have continued until 200-500 Ma. Therefore it may be the youngest dwarf spheroidal satellite galaxy of the Milky Way. In addition, the galaxy may be embedded in a cloud of ionized gas with a mass similar to that of the whole galaxy.[5][7]

Globular clusters

No globular clusters have been found in the galaxy.[5]


Leo I is located only 12 arc minutes from Regulus, the brightest star in the constellation. For that reason, the galaxy is sometimes called the Regulus Dwarf. Scattered light from the star makes studying the galaxy more difficult, and it was not until the 1990s that it was detected visually.[4][5]


  1. ^ a b c d e f g h i j k l "NASA/IPAC Extragalactic Database". Results for Leo I. Retrieved 2006-11-29. 
  2. ^ I. D. Karachentsev, V. E. Karachentseva, W. K. Hutchmeier, D. I. Makarov (2004). "A Catalog of Neighboring Galaxies". Astronomical Journal 127 (4): 2031–2068.  
  3. ^ Karachentsev, I. D.; Kashibadze, O. G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics 49 (1): 3–18.  
  4. ^ a b "Leo I". SEDS Messier Database. Retrieved 2006-05-15. 
  5. ^ a b c d e f Van den Bergh, Sidney (2000). Galaxies of the Local Group (1st ed.). Cambridge University Press. pp. 243–245.  
  6. ^ "Faint Fuzzy Observations". Retrieved 2014-03-24. 
  7. ^  

External links

  • Leo I (dwarf galaxy) on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
  • Astronomy Picture of the Day - Leo I
  • SEDS page on Leo I

This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.

Copyright © World Library Foundation. All rights reserved. eBooks from World eBook Library are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.