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1565 Lemaître

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1565 Lemaître
Discovery [1]
Discovered byS. Arend
Discovery siteUccle – Belgium
Discovery date25 November 1948
Designations
1565 Lemaitre
Named after
Georges Lemaître
(astronomer, priest)[2]
1948 WA
Mars-crosser · Phocaea[3]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc67.40 yr (24617 days)
Aphelion3.2264 AU (482.66 Gm)
Perihelion1.5620 AU (233.67 Gm)
2.3942 AU (358.17 Gm)
Eccentricity0.34757
3.70 yr (1353.1 d)
130.05°
0° 15m 57.78s / day
Inclination21.457°
261.31°
116.09°
Earth MOID0.674365 AU (100.8836 Gm)
Jupiter MOID2.55644 AU (382.438 Gm)
TJupiter3.357
Physical characteristics
Dimensions8.00±0.58 km[4]
8.76 km (calculated)[3]
11.403 h (0.4751 d)[1][5]
2.4±0.1 h[6]
0.334±0.051[4]
0.23 (assumed)[3]
SMASS = Sq
S[3]
12.5

1565 Lemaître, provisional designation 1948 WA, is an eccentric, stony asteroid and sizable Mars-crosser from the inner regions of the asteroid belt, about 8 kilometers in diameter. It was discovered by Belgian astronomer Sylvain Arend at the Royal Observatory of Belgium in Uccle, on 25 November 1948.[7]

The S-type asteroid, classified as a Sq-subtype in the SMASS taxonomy, is a member of the Phocaea family. It orbits the Sun at a distance of 1.6–3.2 AU once every 3 years and 8 months (1,352 days). Its orbit shows an eccentricity of 0.35 and is tilted by 21 degrees to the plane of the ecliptic. It has a rotation period of 11.4 hours[5] and an albedo of 0.33 and 0.23, based on results from the Japanese Akari survey and on assumptions made by the Collaborative Asteroid Lightcurve Link, respectively.[3][4]

The minor planet was named in honour of Belgian priest, astronomer and professor of physics, Georges Lemaître (1894–1966), widely regarded as the father of the Big Bang theory. The lunar crater Lemaître also bears his name. The asteroid 1565 Lemaître was the first minor planet to be numbered after the end of World War II.[2]

References

  1. ^ a b c "JPL Small-Body Database Browser: 1565 Lemaitre (1948 WA)" (2015-09-24 last obs.). Jet Propulsion Laboratory. Retrieved 27 April 2016.
  2. ^ a b Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1565) Lemaître. Springer Berlin Heidelberg. p. 124. ISBN 978-3-540-29925-7. Retrieved November 2015. {{cite book}}: Check date values in: |accessdate= (help)
  3. ^ a b c d e "LCDB Data for (1565) Lemaitre". Asteroid Lightcurve Database (LCDB). Retrieved November 2015. {{cite web}}: Check date values in: |accessdate= (help)
  4. ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved November 2015. {{cite journal}}: Check date values in: |access-date= (help)
  5. ^ a b Warner, Brian D.; Vander Haagen, Gary A. (June 2008). "Lightcurve Analysis of 1565 Lemaitre". The Minor Planet Bulletin. 35 (2): 52. Bibcode:2008MPBu...35...52W. ISSN 1052-8091. Retrieved November 2015. {{cite journal}}: Check date values in: |access-date= (help)
  6. ^ Behrend, Raoul. "Asteroids and comets rotation curves – (1565) Lemaitre". Geneva Observatory. Retrieved November 2015. {{cite web}}: Check date values in: |accessdate= (help)
  7. ^ "1565 Lemaitre (1948 WA)". Minor Planet Center. Retrieved November 2015. {{cite web}}: Check date values in: |accessdate= (help)