Astronomy:571 Dulcinea
From HandWiki
Discovery | |
---|---|
Discovered by | Paul Götz |
Discovery site | Heidelberg |
Discovery date | 4 September 1905 |
Designations | |
(571) Dulcinea | |
Pronunciation | /dʌlˈsɪniə, dʌlsɪˈniːə/[1] |
1905 QZ | |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 110.57 yr (40387 d) |
|{{{apsis}}}|helion}} | 2.9963 astronomical unit|AU (448.24 Gm) |
|{{{apsis}}}|helion}} | 1.8224 AU (272.63 Gm) |
2.4093 AU (360.43 Gm) | |
Eccentricity | 0.24361 |
Orbital period | 3.74 yr (1366.0 d) |
Mean anomaly | 205.094° |
Mean motion | 0° 15m 48.78s / day |
Inclination | 5.2282° |
Longitude of ascending node | 3.1916° |
27.650° | |
Physical characteristics | |
Rotation period | 126.3 h (5.26 d) |
Absolute magnitude (H) | 11.59 |
Dulcinea (minor planet designation: 571 Dulcinea) is an asteroid orbiting in the inner main belt.[3] It was named after Dulcinea, a character from Miguel de Cervantes' novel Don Quixote. This is classified as a stony S-type asteroid and it is the second largest member of the Erigone collisional family.[3]
References
- ↑ Dulcinea (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Dulcinea (Subscription or UK public library membership required.)
- ↑ "571 Dulcinea (1905 QZ)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=571;cad=1.
- ↑ 3.0 3.1 Morate, David et al. (February 2016), "Compositional study of asteroids in the Erigone collisional family using visible spectroscopy at the 10.4 m GTC", Astronomy and Astrophysics 586: 18, doi:10.1051/0004-6361/201527453, A129, Bibcode: 2016A&A...586A.129M.
External links
- 571 Dulcinea at AstDyS-2, Asteroids—Dynamic Site
- 571 Dulcinea at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/571 Dulcinea.
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