27270 Guidotti, provisional designation 2000 AY4, is a carbonaceous background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 2 January 2000, by Italian astronomers Luciano Tesi and Alfredo Caronia at the Pistoia Mountains Astronomical Observatory in San Marcello Pistoiese, Italy.[8] The asteroid was named after amateur astronomer Guido Guidotti.[2]
Discovery [1] | |
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Discovered by | L. Tesi A. Caronia |
Discovery site | San Marcello Obs. |
Discovery date | 2 January 2000 |
Designations | |
MPC designation | (27270) Guidotti |
Named after | Guido Guidotti [2] (Italian amateur astronomer) |
Alternative designations | 2000 AY4 · 1995 YH24 1998 SS103 |
Minor planet category | main-belt · (inner) [3] background [4] |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 25.95 yr (9,479 days) |
Aphelion | 2.6014 AU |
Perihelion | 2.2912 AU |
Semi-major axis | 2.4463 AU |
Eccentricity | 0.0634 |
Orbital period (sidereal) | 3.83 yr (1,398 days) |
Mean anomaly | 142.12° |
Mean motion | 0° 15m 27.36s / day |
Inclination | 2.7846° |
Longitude of ascending node | 107.85° |
Argument of perihelion | 95.008° |
Physical characteristics | |
Mean diameter | 3.74 km (calculated)[3] 6.9 km (est. at 0.06)[5] |
Synodic rotation period | 2.6 h[6] |
Geometric albedo | 0.20 (assumed)[3] |
Spectral type | C [7] · C (SDSS-MFB)[3] |
Absolute magnitude (H) | 14.46±0.28[7] · 14.5[1][3] |
Guidotti is a non-family from the main belt's background population.[4] It orbits the Sun in the inner asteroid belt at a distance of 2.3–2.6 AU once every 3 years and 10 months (1,398 days). Its orbit has an eccentricity of 0.06 and an inclination of 3° with respect to the ecliptic.[1]
The body's observation arc begins with a precovery from the Digitized Sky Survey taken at Palomar Observatory in October 1991, more than 8 years prior to its official discovery observation at San Marcello in 2000.[8]
Guidotti has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey,[7] as well as by SDSS-MFB (Masi Foglia Bus).[3]
In March 2008, a rotational lightcurve of Guidotti was obtained from photometric observations by Slovak astronomers Adrian Galad and Leonard Kornoš. Analysis of the fragmentary lightcurve gave a rotation period of 2.6 hours with a brightness amplitude of 0.3 magnitude (U=1).[6] As of 2017, no secure period has been obtained.[3]
Guidotti has not been observed by any of the spaced-based surveys such as the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the Japanese Akari satellite or the Infrared Astronomical Satellite.
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.74 kilometers based on an absolute magnitude of 14.5.[3] Based on a generic magnitude-to diameter conversion, using a typical albedo for carbonaceous asteroids of 0.06, Guidotti measures 6.9 kilometers in diameter.[5]
This minor planet was named after Guido Guidotti (born 1946), an Italian amateur astronomer and founder of the Association of Astronomy "A. Pieri" (Italian: Associazione Astrofili Valdinievole "A. Pieri"), in Valdinievole, Tuscany, Italy. He is an observer of asteroids and comets, and organizer of lectures and exhibitions on astronomical subjects.[2] The official naming citation was published by the Minor Planet Center on 26 November 2004 (M.P.C. 53176).[9]
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