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1301 Yvonne
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Main-belt asteroid
October 2019
yes
1301 Yvonne
#D6D6D6
001301-asteroid shape model (1301) Yvonne.png
Modelled shape of Yvonne from its lightcurve
L. Boyer
Algiers Obs.
7 March 1934
(1301) Yvonne
1934 EA
Yvonne Boyer(discoverer's sister)
main-belt(outer)background
4 September 2017 (JD 2458000.5)
0
83.32 yr (30,433 days)
3.5134 AU
2.0225 AU
2.7680 AU
0.2693
4.61 yr (1,682 days)
96.456°
0.2140 ms / day
34.030°
161.56°
302.27°
18.693 4.943 km20.44 5.24 km21.438 0.088 km21.54 0.25 km21.681 0.204 km21.95 0.41 km22.77 2.4 km
7.2536 0.0002 h7.3196 0.0001 h7.3200 0.0001 h7.320 0.005 h
(39.0°, 41.0°) (λ1/β1)
0.10 0.120.111 0.0200.1167 0.07000.1632 0.0400.1806 0.04790.201 0.006
SMASS CC
10.8011.3011.3211.40 0.22
1301 Yvonne (prov. designation: 1934 EA) is a carbonaceous background asteroid from the background population of the intermediate asteroid belt, approximately 21 km mi off 2 us in diameter. It was discovered on 7 March 1934, by French astronomer Louis Boyer at the Algiers Observatory in North Africa. The asteroid was named for the discoverer's sister, Yvonne Boyer
Orbit and classification
Yvonne is a non-family of the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.0–3.5 AU once every 4 years and 7 months (1,682 days; semi-major axis of 2.77 AU). Its orbit has an eccentricity of 0.27 and an inclination of 34° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Algiers in March 1934.
Naming
This minor planet was named after Yvonne Boyer, sister of discoverer. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 101).
Physical characteristics
In the SMASS classification, Yvonne is a carbonaceous C-type asteroid. PanSTARRS photometric survey also characterized the asteroid as a C-type.
Rotation period and pole
thumb|left|265px|Lightcurve-based 3D-model of Yvonne
Between 2003 and 2017, four rotational lightcurves of Yvonne have been obtained from photometric observations. Analysis gave a consolidated rotation period of 7.320 hours with a brightness amplitude between 0.52 and 0.90 magnitude (U=3/3/3/3). In 2011, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue (UAPC) and other sources gave a concurring period 7.31968 0.00005 hours, as well as a spin axis of (39.0°, 41.0°) in ecliptic coordinates (λ, β).
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Yvonne measures between 18.693 and 22.77 kilometers in diameter and its surface has an albedo between 0.10 and 0.201.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1054 (which is untypically high for a carbonaceous body) and a diameter of 22.50 kilometers based on an absolute magnitude of 11.3.
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30em 2017-07-02 last obs.
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1301 Yvonne (1934 EA)
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11 December 2017
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External links
Lightcurve Database Query (LCDB), at www.minorplanet.info
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1301
1300 Marcelle 1301 1302 Werra
001301
Category:Discoveries by Louis Boyer (astronomer)
Category:Named minor planets
001301
19340307