Equuleus: Difference between revisions
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The brightest star in Equuleus is [[Alpha Equulei]], traditionally called Kitalpha, a yellow star magnitude 3.9, 186 light-years from Earth. Its traditional name means "the section of the horse".{{sfn|Ridpath|Tirion|2001|pp=144-145}} |
The brightest star in Equuleus is [[Alpha Equulei]], traditionally called Kitalpha, a yellow star magnitude 3.9, 186 light-years from Earth. Its traditional name means "the section of the horse".{{sfn|Ridpath|Tirion|2001|pp=144-145}} |
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There are few [[variable star]]s in Equuleus. Only around 25 are known, most of which are faint. [[Gamma Equulei]] is an [[alpha CVn star]], ranging between magnitudes 4.58 and 4.77 over a period of around 12½ minutes.<!-- not cited to Ridpath and Tirion 2001 --> It is a white star 115 light-years from Earth, and has an [[optical binary|optical companion]] of magnitude 6.1, [[6 Equulei]]. It is divisible in binoculars.{{sfn|Ridpath|Tirion|2001|pp=144-145}} [[R Equulei]] is a [[Mira variable]] that ranges between magnitudes 8.0 and 15.7 over nearly 261 days. |
There are few [[variable star]]s in Equuleus. Only around 25 are known, most of which are faint. [[Gamma Equulei]] is an [[alpha CVn star]], ranging between magnitudes 4.58 and 4.77<ref>{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}</ref> over a period of around 12½ minutes.<!-- not cited to Ridpath and Tirion 2001 --> It is a white star 115 light-years from Earth, and has an [[optical binary|optical companion]] of magnitude 6.1, [[6 Equulei]]. It is divisible in binoculars.{{sfn|Ridpath|Tirion|2001|pp=144-145}} [[R Equulei]] is a [[Mira variable]] that ranges between magnitudes 8.0 and 15.7 over nearly 261 days. |
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Equuleus contains some [[double star]]s of interest. γ Equ consists of a primary star with a magnitude around 4.7 (slightly variable) and a secondary star of magnitude 11.6, separated by 2 [[arcsecond]]s. [[Epsilon Equulei]] is a triple star also designated 1 Equulei. The system, 197 light-years away, has a primary of magnitude 5.4 that is itself a binary star; its components are of magnitude 6.0 and 6.3 and have a period of 101 years. The secondary is of magnitude 7.4 and is visible in small telescopes. The components of the primary are becoming closer together and will not be divisible in amateur telescopes beginning in 2015.{{sfn|Ridpath|Tirion|2001|pp=144-145}} [[Delta Equulei|δ Equ]] is a [[binary star]] with an orbital period of 5.7 years, which at one time was the shortest known orbital period for an optical binary. The two components of the system are never more than 0.35 arcseconds apart. |
Equuleus contains some [[double star]]s of interest. γ Equ consists of a primary star with a magnitude around 4.7 (slightly variable) and a secondary star of magnitude 11.6, separated by 2 [[arcsecond]]s. [[Epsilon Equulei]] is a triple star also designated 1 Equulei. The system, 197 light-years away, has a primary of magnitude 5.4 that is itself a binary star; its components are of magnitude 6.0 and 6.3 and have a period of 101 years. The secondary is of magnitude 7.4 and is visible in small telescopes. The components of the primary are becoming closer together and will not be divisible in amateur telescopes beginning in 2015.{{sfn|Ridpath|Tirion|2001|pp=144-145}} [[Delta Equulei|δ Equ]] is a [[binary star]] with an orbital period of 5.7 years, which at one time was the shortest known orbital period for an optical binary. The two components of the system are never more than 0.35 arcseconds apart. |
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Revision as of 17:55, 22 July 2022
| Constellation | |
 | |
| Abbreviation | Equ |
|---|---|
| Genitive | Equulei |
| Pronunciation | /ɪˈkwuːliəs/ Equúleus, genitive /ɪˈkwuːliaɪ/ |
| Symbolism | the pony |
| Right ascension | 21h |
| Declination | +10° |
| Quadrant | NQ4 |
| Area | 72 sq. deg. (87th) |
| Main stars | 3 |
| Bayer/Flamsteed stars | 10 |
| Stars with planets | 2 |
| Stars brighter than 3.00m | 0 |
| Stars within 10.00 pc (32.62 ly) | 0 |
| Brightest star | α Equ (Kitalpha) (3.92m) |
| Messier objects | 0 |
| Meteor showers | 0 |
| Bordering constellations | Aquarius Delphinus Pegasus |
| Visible at latitudes between +90° and −80°. Best visible at 21:00 (9 p.m.) during the month of September. | |
Equuleus (/ɪˈkwuːliəs/ ih-KWOO-lee-əs) is a constellation of stars that are visible in the night sky. Its name is Latin for "little horse", a foal. Located on the northern celestial hemisphere, it was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is the second smallest of the modern constellations (after Crux), spanning only 72 square degrees. It is also very faint, having no stars brighter than the fourth magnitude.
Notable features
Stars
The brightest star in Equuleus is Alpha Equulei, traditionally called Kitalpha, a yellow star magnitude 3.9, 186 light-years from Earth. Its traditional name means "the section of the horse".[1]
There are few variable stars in Equuleus. Only around 25 are known, most of which are faint. Gamma Equulei is an alpha CVn star, ranging between magnitudes 4.58 and 4.77[2] over a period of around 12½ minutes. It is a white star 115 light-years from Earth, and has an optical companion of magnitude 6.1, 6 Equulei. It is divisible in binoculars.[1] R Equulei is a Mira variable that ranges between magnitudes 8.0 and 15.7 over nearly 261 days.
Equuleus contains some double stars of interest. γ Equ consists of a primary star with a magnitude around 4.7 (slightly variable) and a secondary star of magnitude 11.6, separated by 2 arcseconds. Epsilon Equulei is a triple star also designated 1 Equulei. The system, 197 light-years away, has a primary of magnitude 5.4 that is itself a binary star; its components are of magnitude 6.0 and 6.3 and have a period of 101 years. The secondary is of magnitude 7.4 and is visible in small telescopes. The components of the primary are becoming closer together and will not be divisible in amateur telescopes beginning in 2015.[1] δ Equ is a binary star with an orbital period of 5.7 years, which at one time was the shortest known orbital period for an optical binary. The two components of the system are never more than 0.35 arcseconds apart.
Deep-sky objects
Due to its small size and its distance from the plane of the Milky Way, Equuleus contains no notable deep sky objects. Some very faint galaxies between magnitudes 13 and 15 include NGC 7015, NGC 7040, NGC 7045 and NGC 7046.
![[icon]](/enwiki/wiki/File:Wiki_letter_w_cropped.svg){kind=small} | This section needs expansion. You can help by adding to it. (June 2008) |
Mythology
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In Greek mythology, one myth associates Equuleus with the foal Celeris (meaning "swiftness" or "speed"), who was the offspring or brother of the winged horse Pegasus. Celeris was given to Castor by Mercury. Other myths say that Equuleus is the horse struck from Poseidon's trident, during the contest between him and Athena when deciding which would be the superior. Because this section of stars rises before Pegasus, it is often called Equus Primus, or the First Horse. Equuleus is also linked to the story of Philyra and Saturn.[3]
Created by Hipparchus and included by Ptolemy, it abuts Pegasus; unlike the larger horse it is depicted as a horse's head alone.[1] [4]
Equivalents
In Chinese astronomy, the stars that correspond to Equuleus are located within the Black Tortoise of the North (北方玄武, Běi Fāng Xuán Wǔ).[5]
In fiction
Equuleus is briefly mentioned in the Martha Speaks episode "Dogs in Space" as one of Helen Lorraine's favorite constellations.
See also
References
- Burnham, Robert (1978). Burnham's Celestial Handbook: An observer's guide to the universe beyond the solar system, vol 2. Dover Publications ISBN 0-486-23567-X
- Hoffleit+ (1991) V/50 The Bright Star Catalogue, 5th revised ed, Yale University Observatory, Strasbourg astronomical Data Center
- Ridpath, Ian; Tirion, Wil (2001), Stars and Planets Guide, Princeton University Press, ISBN 0-691-08913-2
- Ian Ridpath & Wil Tirion (2007). Stars and Planets Guide, Collins, London. ISBN 978-0-00-725120-9. Princeton University Press, Princeton. ISBN 978-0-691-13556-4.
- ^ a b c d Ridpath & Tirion 2001, pp. 144–145.
- ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
- ^ Olcott, William Tyler (2004). Star lore of all ages : myths, legends, and facts. Fred Schaaf (Dover ed.). Mineola, N.Y.: Dover Publications. p. 297. ISBN 978-0-486-14080-3. OCLC 947036847.
- ^ Evans, James "The History and Practice of Ancient Astronomy" Oxford University Press, 1998.
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 15 日
External links
- The Deep Photographic Guide to the Constellations: Equuleus
- The clickable Equuleus
- Star Tales – Equuleus
- Warburg Institute Iconographic Database (medieval and early modern images of Equuleus)
