2598 Merlin
Template:Short description Template:DMCA
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| Discovery[1] | |
|---|---|
| Discovered by | E. Bowell |
| Discovery site | Anderson Mesa Stn. |
| Discovery date | 7 September 1980 |
| Designations | |
Named after | Merlin (Arthurian legend)[2] |
| 1980 RY · 1948 WH Template:Mp | |
| main-belt · Dora[3] | |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 68.44 yr (24,998 days) |
| Aphelion | 3.3861 AU |
| Perihelion | 2.1757 AU |
| 2.7809 AU | |
| Eccentricity | 0.2176 |
| 4.64 yr (1,694 days) | |
| 297.39° | |
| Template:Deg2DMS / day | |
| Inclination | 7.7767° |
| 197.77° | |
| 217.28° | |
| Physical characteristics | |
| Dimensions | 15.694±0.047 km[4] |
| 0.049±0.010[4] | |
| SMASS = Ch[1] | |
| 13.2[1] | |
| Page Template:Reflist/styles.css has no content. | |
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2598 Merlin, provisional designation Template:Mp, is a carbonaceous Dorian asteroid from the central regions of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 7 September 1980, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona, United States.[5] The asteroid was named after the legendary wizard Merlin in Arthurian legend.[2]
Classification and orbit
Merlin is a member of the Dora family (512), a well-established central asteroid family of more than 1,200 carbonaceous asteroids. The family's namesake is 668 Dora. It is alternatively known as the "Zhongolovich family", named after its presumably largest member 1734 Zhongolovich. The Dora family may also contain a subfamily.[3][6]Template:Rp
Merlin orbits the Sun in the central main-belt at a distance of 2.2–3.4 AU once every 4 years and 8 months (1,694 days). Its orbit has an eccentricity of 0.22 and an inclination of 8° with respect to the ecliptic.[1] In Nombember 1948, the asteroid was first identified Template:Mp at Uccle Observatory, where the body's observation arc begins 32 years prior to its official discovery observation at Anderson Mesa.[5]
Physical characteristics
In the SMASS classification, Merlin a Ch-type asteroid, a hydrated subtype of the broader carbonaceous C-complex.[1]
According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Merlin measures 15.694 kilometers in diameter and its surface has an albedo of 0.049.[4]
Lightcurves
As of 2017, no rotational lightcurve of Merlin has been obtained from photometric observations. The body's rotation period and shape remain unknown.[1][7]
Naming
This minor planet was named after the sage and sorcerer Merlin, featured mentor of King Arthur in Arthurian legend and medieval Welsh poetry. His magic enabled Arthur to pull Excalibur from the rock and become the rightwise king born of all England. The name was suggested by F. Pilcher.[2] The approved naming citation was published by the Minor Planet Center on 4 August 1982 (M.P.C. 7157).[8]
Notes
There is a book titled Merlin's Tour of the Universe, in which a fictitious character, called Merlin, answers all curious questions a layman would have about astronomy and the Solar System. In the book, Merlin's favorite asteroid is Merlin 2598.
References
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- ^ a b c d e f g Page Module:Citation/CS1/styles.css has no content."JPL Small-Body Database Browser: 2598 Merlin (1980 RY)" (2017-05-05 last obs.). Jet Propulsion Laboratory. Retrieved 7 July 2017.
- ^ a b c Page Module:Citation/CS1/styles.css has no content.Schmadel, Lutz D. (2007). "(2598) Merlin". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 212. doi:10.1007/978-3-540-29925-7_2599. ISBN 978-3-540-00238-3.
- ^ a b Page Module:Citation/CS1/styles.css has no content.Broz, M.; Morbidelli, A.; Bottke, W. F.; Rozehnal, J.; Vokrouhlický, D.; Nesvorný, D. (March 2013). "Constraining the cometary flux through the asteroid belt during the late heavy bombardment". Astronomy and Astrophysics. 551: 16. arXiv:1301.6221. Bibcode:2013A&A...551A.117B. doi:10.1051/0004-6361/201219296.
- ^ a b c Page Module:Citation/CS1/styles.css has no content.Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 7 July 2017.
- ^ a b Page Module:Citation/CS1/styles.css has no content."2598 Merlin (1980 RY)". Minor Planet Center. Retrieved 7 July 2017.
- ^ Page Module:Citation/CS1/styles.css has no content.Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 978-0-8165-3213-1.
- ^ Template:Cite LCDB
- ^ Page Module:Citation/CS1/styles.css has no content."MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 July 2017.
External links
- Asteroid Lightcurve Database (LCDB), query form (info Script error: No such module "webarchive".)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- Template:AstDys
- 2598 Merlin at the JPL Small-Body DatabaseTemplate:Edit at Wikidata
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