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4282 Endate

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Asteroid from the inner regions of the asteroid belt
4282 Endate
Discovery 
Discovered byS. Ueda
H. Kaneda
Discovery siteKushiro Obs. (399)
Discovery date28 October 1987
Designations
MPC designation(4282) Endate
Named afterKin Endate
(amateur astronomer)
Alternative designations1987 UQ1 · 1959 EJ
1983 RT
Minor planet categorymain-belt · (inner) 
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc61.89 yr (22,605 days)
Aphelion2.7389 AU
Perihelion2.0449 AU
Semi-major axis2.3919 AU
Eccentricity0.1451
Orbital period (sidereal)3.70 yr (1,351 days)
Mean anomaly6.4722°
Mean motion0° 15 59.04 / day
Inclination2.7202°
Longitude of ascending node325.81°
Argument of perihelion101.31°
Physical characteristics
Dimensions5.66 km (calculated)
7.386±1.581 km
11.52±3.27 km
12.12±0.49 km
13.73±7.43 km
Synodic rotation period34 h
Geometric albedo0.038±0.050
0.04±0.02
0.058±0.005
0.13±0.08
0.20 (assumed)
Spectral typeS
Absolute magnitude (H)13.30 · 13.48 · 13.50 · 13.6 · 13.93

4282 Endate, provisional designation 1987 UQ1, is an asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 28 October 1987, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at Kushiro Observatory (399) in Japan. It was named for amateur astronomer Kin Endate.

Orbit and classification

Endate is a presumed stony S-type asteroid. It orbits the Sun in the inner main-belt at a distance of 2.0–2.7 AU once every 3 years and 8 months (1,351 days). Its orbit has an eccentricity of 0.15 and an inclination of 3° with respect to the ecliptic. The first precovery was taken at Palomar Observatory in 1954, extending the body's observation arc by 33 years prior to its official discovery observation.

Physical characteristics

Rotation period

In April 2014, a rotational lightcurve of Endate was obtained from photometric observations by Hungarian astronomer Gyula M. Szabó. Lightcurve analysis gave it a longer-than average rotation period of 34 hours with a brightness amplitude of 0.5 magnitude (U=n.a.). Most minor planets have a spin rate between 2 and 20 hours. Endate's rotation period is significantly longer but still much shorter than that of the so-called slow rotators, which take at least 100 hours to rotate once around their axis.

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Endate measures between 7.386 and 13.73 kilometers in diameter and its surface has an albedo between 0.038 and 0.15. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a smaller diameter of 5.66 kilometers.

Naming

This minor planet was named in honor of Japanese amateur astronomer Kin Endate from Bihoro in northern Japan. He is a prolific observer and discoverer of minor planets. The official naming citation was published by the Minor Planet Center on 8 July 1990 (M.P.C. 16593).

References

  1. ^ "JPL Small-Body Database Browser: 4282 Endate (1987 UQ1)" (2016-11-11 last obs.). Jet Propulsion Laboratory. Archived from the original on 12 March 2017. Retrieved 20 June 2017.
  2. ^ Schmadel, Lutz D. (2007). "(4282) Endate". Dictionary of Minor Planet Names – (4282) Endate. Springer Berlin Heidelberg. p. 367. doi:10.1007/978-3-540-29925-7_4242. ISBN 978-3-540-00238-3.
  3. ^ "LCDB Data for (4282) Endate". Asteroid Lightcurve Database (LCDB). Retrieved 9 March 2017.
  4. ^ Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID 9341381. Retrieved 9 March 2017.
  5. ^ Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63.
  6. ^ 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. (online, AcuA catalog p. 153)
  7. ^ Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317. Retrieved 9 March 2017.
  8. ^ "4282 Endate (1987 UQ1)". Minor Planet Center. Retrieved 9 March 2017.
  9. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 9 March 2017.

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