Equuleus

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Equuleus
Constellation
Equuleus IAU.svg
List of stars in Equuleus
AbbreviationEqu
Genitive Equulei
Pronunciation /ɪˈkwuːliəs/ Equúleus, genitive /ɪˈkwuːliaɪ/
Symbolismthe pony
Right ascension 20h 56m 10.9212s–21h 26m 20.0331s [1]
Declination 13.0390635°–2.4773185° [1]
QuadrantNQ4
Area 72 sq. deg. (87th)
Main stars 3
Bayer/Flamsteed
stars		10
Stars with planets 2
Stars brighter than 3.00m0
Stars within 10.00 pc (32.62 ly)0
Brightest star α Equ (Kitalpha) (3.92 m )
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 is a faint constellation located just north of the celestial equator. Its name is Latin for "little horse", a foal. 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.

Contents

Notable features

The constellation Equuleus as it can be seen by the naked eye. EquuleusCC.jpg
The constellation Equuleus as it can be seen by the naked eye.
The constellation Equuleus, color and contrast enhanced. Equuleus 20191202.jpg
The constellation Equuleus, color and contrast enhanced.

Stars

The brightest star in Equuleus is α Equulei, traditionally called Kitalpha, a yellow star magnitude 3.9, 186 light-years from Earth. Its traditional name means "the section of the horse". [2]

There are few variable stars in Equuleus. Only around 25 are known, most of which are faint. γ Equulei is an α2 CVn variable star, ranging between magnitudes 4.58 and 4.77 [3] 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. [2] 6 Equulei is an astrometric binary system itself, [4] with an apparent magnitude of 6.07. [5] R Equulei is a Mira variable that ranges between magnitudes 8.0 and 15.7 [6] over nearly 261 days. It has a spectral type of M3e-M4e [6] and has an average B-V colour index of +1.41. [7]

Equuleus contains some double stars of interest. γ Equulei 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. ε 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. [2] δ Equulei 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 is rather devoid of deep sky objects. Some very faint galaxies in the NGC catalog between magnitudes 13 and 15 include NGC 7015, NGC 7040, and NGC 7046. NGC 7045 is a triple star that was mistaken as a nebula by its discoverer, John Herschel. [8] Other faint galaxies in the IC Catalog include IC 1360, IC 1361, IC 1364, IC 1367, IC 1375, and IC 5083. IC 1365 is a group of galaxies. The magnitudes of these objects vary from 14.5 to 15.5, making them hard to see in even the largest of amateur telescopes. [9]

Mythology

Seen in Urania's Mirror (1825) Sidney Hall - Urania's Mirror - Pegasus and Equuleus (best currently available version - 2014).jpg
Seen in Urania's Mirror (1825)

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. [10]

Created by Hipparchus and included by Ptolemy, it abuts Pegasus; unlike the larger horse, it is depicted as a horse's head alone. [2] [11]

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). [12]

See also

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<span class="mw-page-title-main">12 Vulpeculae</span> Star in the constellation Vulpecula

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<span class="mw-page-title-main">HD 155035</span> Star in the constellation Ara

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<span class="mw-page-title-main">S Pegasi</span> Variable star in the constellation Pegasus

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<span class="mw-page-title-main">Gamma Equulei</span> Chemically peculiar A-type main sequence star in the constellation Equuleus

Gamma Equulei, Latinized from γ Equulei, is a double star in the northern constellation of Equuleus. It is located at a distance of around 118 light-years from Earth and is visible to the naked eye with a slightly variable apparent visual magnitude of around 4.7. The star is drifting closer to the Sun with a radial velocity of −16.5 km/s.

9 Equulei is an M-type star in the constellation Equuleus. It is an asymptotic giant branch (AGB) star, a star that has exhausted its core helium and is now fusing both hydrogen and helium in shells outside the core. It is also a suspected variable star with an amplitude of about 0.05 magnitudes.

<span class="mw-page-title-main">R Equulei</span> Variable star in the constellation of Equuleus

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<span class="mw-page-title-main">42 Persei</span> Binary star system in the constellation Perseus

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<span class="mw-page-title-main">3 Geminorum</span> Star in the constellation Gemini

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<span class="mw-page-title-main">HO Telescopii</span> Star in the constellation Telescopium

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References

  1. 1 2 IAU, The Constellations, Equuleus.
  2. 1 2 3 4 Ridpath & Tirion 2001, pp. 144–145.
  3. ↑ 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.
  4. ↑ Frankowski, A.; Jancart, S.; Jorissen, A. (March 2007), "Proper-motion binaries in the Hipparcos catalogue. Comparison with radial velocity data", Astronomy and Astrophysics, 464 (1): 377–392, arXiv: astro-ph/0612449 , Bibcode:2007A&A...464..377F, doi:10.1051/0004-6361:20065526, S2CID   14010423
  5. ↑ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99, Bibcode:1966CoLPL...4...99J
  6. 1 2 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: B/gcvs, Bibcode:2009yCat....102025S.
  7. ↑ Zacharias, N.; et al. (2012), "The fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)", VizieR On-line Data Catalog, 1322 (2): 44, arXiv: 1212.6182 , Bibcode:2012yCat.1322....0Z, doi:10.1088/0004-6256/145/2/44, S2CID   119299381.
  8. ↑ "NGC 7045 Basic Information". The NGC/IC Project. Retrieved 2024-03-25.
  9. ↑ "Deep sky objects in Equuleus - Full list". The Sky Live. Retrieved 2024-03-25.
  10. ↑ 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.
  11. ↑ Evans, James "The History and Practice of Ancient Astronomy" Oxford University Press, 1998.
  12. ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 15 日
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