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===Deep sky objects=== |
===Deep sky objects=== |
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Faggit :) |
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The brightest deep sky object in Leo Minor is NGC 3003, a galaxy with an apparent brightness of 11.7m and an angular size of 5.9 arcminutes. It is seen almost edge-on. |
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The mysterious deep sky object known as [[Hanny's Voorwerp]] was discovered here in 2007 by Dutch school teacher Hanny van Arkel while participating as a volunteer in the [[Galaxy Zoo]] project. |
The mysterious deep sky object known as [[Hanny's Voorwerp]] was discovered here in 2007 by Dutch school teacher Hanny van Arkel while participating as a volunteer in the [[Galaxy Zoo]] project. |
Revision as of 16:40, 2 October 2009
Constellation | |
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Abbreviation | LMi |
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Genitive | Leonis Minoris |
Pronunciation | /ˌliːoʊ ˈmaɪnər/, genitive /liːˈoʊnɨs mɨˈnɒrɨs/ |
Right ascension | 10 |
Declination | +35 |
Area | 232 sq. deg. (64th) |
Main stars | 2 |
Bayer/Flamsteed stars | 34 |
Stars with planets | 1 |
Stars brighter than 3.00m | 0 |
Stars within 10.00 pc (32.62 ly) | 2 |
Brightest star | 46 LMi (Praecipua) (3.83m) |
Messier objects | 0 |
Bordering constellations | Ursa Major Lynx Cancer (corner) Leo |
Visible at latitudes between +90° and −45°. Best visible at 21:00 (9 p.m.) during the month of April. |
Leo Minor is a small and faint constellation. Its name means "the smaller lion", in contrast to Leo, the larger lion. Its brightest stars form a rough triangle, and it lies between the larger and more recognizable Ursa Major and Leo. Leo Minor was not regarded as a separate constellation by the ancients; it was created by Johannes Hevelius in 1687.
Notable features
![](http://upload.wikimedia.org/wikipedia/commons/0/02/Leourania.jpg)
Leo Minor contains little to see with small telescopes.
Stars
There is only one star brighter than fourth magnitude.
- 46 LMi (Praecipua): an almost (but not quite) giant star of spectral class K0 which lies at a distance of approximately 98 light years and sports an apparent brightness of 3.83. Praecipua does not have a Bayer designation, making Leo Minor the only constellation whose brightest star does not have one.
- β LMi: strangely enough this giant star of spectral class G8 is the only star with a Bayer designation, and with its apparent magnitude of 4.21 it is not even the brightest star of Leo Minor.
- R LMi: this cool long-period variable star (a Mira variable) varies between magnitudes 6.3 and 13.2 during a period of 372.19 days.
- 20 LMi: this binary star system is only 14.9 parsecs away from the Sun.
Deep sky objects
Faggit :)
The mysterious deep sky object known as Hanny's Voorwerp was discovered here in 2007 by Dutch school teacher Hanny van Arkel while participating as a volunteer in the Galaxy Zoo project.
See also
References
- Ian Ridpath and Wil Tirion (2007). Stars and Planets Guide, Collins, London. ISBN 978-0007251209. Princeton University Press, Princeton. ISBN 978-0691135564.
External links
![](http://upload.wikimedia.org/wikipedia/en/thumb/4/4a/Commons-logo.svg/30px-Commons-logo.svg.png)
Wikimedia Commons has media related to Leo Minor.