Delphinus
Constellation | |
Rotanev (β Del) (3.63m) | |
Messier objects | 0 |
---|---|
Meteor showers | None |
Bordering constellations | Vulpecula Sagitta Aquila Aquarius Equuleus Pegasus |
Visible at latitudes between +90° and −69°. Best visible at 21:00 (9 p.m.) during the month of September. |
Delphinus (Pronounced
Delphinus is a faint constellation with only two stars brighter than an apparent magnitude of 4, Beta Delphini (Rotanev) at magnitude 3.6 and Alpha Delphini (Sualocin) at magnitude 3.8.
Mythology
Delphinus is associated with two stories from Greek mythology.
According to myth, the first Greek god
The second story tells of the Greek poet Arion of Lesbos (7th century BC), who was saved by a dolphin.[3] He was a court musician at the palace of Periander, ruler of Corinth. Arion had amassed a fortune during his travels to Sicily and Italy. On his way home from Tarentum his wealth caused the crew of his ship to conspire against him. Threatened with death, Arion asked to be granted a last wish which the crew granted: he wanted to sing a dirge.[4] This he did, and while doing so, flung himself into the sea. There, he was rescued by a dolphin which had been charmed by Arion's music. The dolphin carried Arion to the coast of Greece and left.[5]
In non-Western astronomy
In
In Polynesia, two cultures recognized Delphinus as a constellation. In Pukapuka, it was called Te Toloa and in the Tuamotus, it was called Te Uru-o-tiki.[7]
In Hindu astrology, the Delphinus corresponds to the Nakshatra, or lunar mansion, of Dhanishta.
Characteristics
Delphinus is bordered by Vulpecula to the north, Sagitta to the northwest, Aquila to the west and southwest, Aquarius to the southeast, Equuleus to the east and Pegasus to the east.[1] Covering 188.5 square degrees, corresponding to 0.457% of the sky, it ranks 69th of the 88 constellations in size.[8] The three-letter abbreviation for the constellation, as adopted by the IAU in 1922, is "Del".[9] The official constellation boundaries, as set by Eugène Delporte in 1930, are defined by a polygon of 14 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 20h 14m 14.1594s and 21h 08m 59.6073s, while the declination coordinates are between +2.4021468° and +20.9399471°.[1] The whole constellation is visible to observers north of latitude 69°S.[8][a]
Features
Stars
Delphinus has two stars above fourth (apparent) magnitude; its brightest star is of magnitude 3.6. The main asterism in Delphinus is Job's Coffin, nearly a 45°-apex lozenge or diamond of the four brightest stars: Alpha, Beta, Gamma, and Delta Delphini. Delphinus is in a rich Milky Way star field. Alpha and Beta Delphini have 19th century names Sualocin and Rotanev, read backwards: Nicolaus Venator, the Latinized name of a Palermo Observatory director, Niccolò Cacciatore (d. 1841).[3]
Alpha Delphini is a blue-white hued main sequence star of magnitude 3.8,[10] 241 light-years from Earth. It is a spectroscopic binary.[11] It is officially named Sualocin.[12][13] The star has an absolute magnitude of -0.4.[14]
Beta Delphini is officially called Rotanev.[12] It was found to be a binary star in 1873.[15] The gap between its close binary stars is visible from large amateur telescopes. To the unaided eye, it appears to be a white star of magnitude 3.6.[16][15] It has a period of 27 years and is 97 light-years from Earth.
Gamma Delphini is a celebrated binary star among amateur astronomers. The primary is orange-gold of magnitude 4.3; the secondary is a light yellow star of magnitude 5.1. The pair form a true binary with an estimated orbital period of over 3,000 years. 125 light-years away, the two components are visible in a small amateur telescope.[3] The secondary, also described as green, is 10 arcseconds from the primary. Struve 2725, called the "Ghost Double", is a pair that appears similar but dimmer. Its components of magnitudes 7.6 and 8.4 are separated by 6 arcseconds and are 15 arcminutes from Gamma Delphini itself.[5] An unconfirmed exoplanet with a minimum mass of 0.7 Jupiter masses may orbit one of the stars.[17][18]
Zeta Delphini, an A3Va[25] main-sequence star of magnitude 4.6, was in 2014 discovered to have a brown dwarf orbiting around it. Zeta Delphini B has a mass of 50±15 MJ.[25]
HR Delphini was a nova that brightened to magnitude 3.5 in December 1967.[29] It took an unusually long time for the nova to reach peak brightness which indicate that it barely satisfied the conditions for a thermonuclear runaway.[30] Another nova by the name V339 Delphini was detected in 2013; it peaked at magnitude 4.3 and was the first nova observed to produce lithium.[31][32][33][34]
Deep-sky objects
Its rich Milky Way star field means many modestly deep-sky objects. NGC 6891 is a planetary nebula of magnitude 10.5; another is NGC 6905 or the Blue Flash Nebula. The Blue Flash Nebula shows broad emission lines. The central star in NGC 6905 has a spectral of WO2, meaning it is rich in oxygen.[38]
See also
- Delphinus (Chinese astronomy)
Notes
- 87°S, stars within a few degrees of the horizon are practically unobservable.[8]
Citations
- ^ a b c d "Delphinus, Constellation Boundary". The Constellations. International Astronomical Union. Retrieved 15 July 2020.
- ^ Pseudo-Hyginus. "HYGINUS, ASTRONOMICA 2.1-17". Theoi Classical Texts Library. Retrieved June 26, 2017.
- ^ a b c Ridpath & Tirion 2017, pp. 140–141.
- Shakespeare, Twelfth Night (Act I, Sc 2, line 16)
- ^ Bibcode:2012S&T...124c..47S.
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 4 日
- ^ Makemson 1941, p. 283.
- ^ a b c Ridpath, Ian. "Constellations: Andromeda–Indus". Star Tales. Self-published. Retrieved 4 March 2016.
- Bibcode:1922PA.....30..469R.
- Bibcode:1991A&AS...89..415O.
- .
- ^ ISBN 978-1-931559-44-7.
- ^ "Naming Stars". IAU.org. Retrieved 16 December 2017.
- Bibcode:1998A&A...330..619J.
- ^ ISBN 0-486-23568-8
- S2CID 122194357
- ISBN 1-58381-011-0
- S2CID 16755455.
- doi:10.1086/319956.
- S2CID 118900730.
- .
- doi:10.1086/190179.
- S2CID 125853869.
- doi:10.1086/111220.
- ^ ISSN 0035-8711.
- ^ Bibcode:1999VeARI..35....1W.
- ISBN 978-1-4471-3613-2.
- S2CID 131780028.
- Bibcode:1974JBAA...85...54I.
- Bibcode:1992A&A...262..487F. Retrieved 19 July 2020.
- S2CID 205242345.
- ^ King, Bob (August 14, 2013). "Bright New Nova In Delphinus — You can See it Tonight With Binoculars". Universe Today (initial designation PNV J20233073+2046041). Retrieved August 15, 2013.
- ^ Guido, Ernesto; Ruocco, Nello; Howes, Nick (August 15, 2013). "Possible Bright Nova in Delphinus". Associazione Friulana di Astronomia e Meteorologia. Retrieved August 15, 2013.
- Virtual Telescope Project. Retrieved August 15, 2013.
- Bibcode:1957ArA.....2...55O.
- ISSN 0004-6264.
- ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 19 July 2020.
- .
- S2CID 1232455.
- ^ Bibcode:1927BHarO.849...11S.
- ^ S2CID 16914232.
- S2CID 14431121.
- S2CID 119461759. 81.
References
- Makemson, Maud Worcester (1941). The Morning Star Rises: an account of Polynesian astronomy. Bibcode:1941msra.book.....M.
- Ridpath, Ian; Tirion, Wil (2017). Stars and planets guide. London: Collins. ISBN 978-0-691-17788-5.
External links
- The Deep Photographic Guide to the Constellations: Delphinus
- The clickable Delphinus
- Star Tales – Delphinus
- Warburg Institute Iconographic Database (medieval and early modern images of Delphinus)