(66391) 1999 KW₄

66391 Moshup
1999kw4 vlt-eso1910.jpg
Moshup and its satellite Squannit imaged by the Very Large Telescope's SPHERE instrument[1]
Discovery [2]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date20 May 1999
Designations
Named after
Moshup
(native American legend)
1999 KW4
Aten · NEO · PHA[2][3]
Mercury-crosser
Venus-crosser
Orbital characteristics[2]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc19.01 yr (6,942 days)
Aphelion1.0845 AU
Perihelion0.2000 AU
0.6422 AU
Eccentricity0.6886
0.51 yr (188 days)
359.03°
1° 54m 54s / day
Inclination38.884°
244.91°
192.62°
Known satellites1 (Squannit)
Earth MOID0.0138 AU · 5.4 LD
Physical characteristics
Dimensions1.532 km × 1.495 km × 1.347 km[4]
Mean diameter
1.317±0.040 km[4]
Mass(2.49±0.054)×1012 kg[4]
2.7650 h[5]
9.581±0.019 h[6]
0.26 (derived)[7]
SMASS = S:[2] · S[7]
16.5[2][7]

66391 Moshup, provisional designation 1999 KW4, is a binary[8] asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Aten group, approximately 1.3 kilometers in diameter. It was discovered on 20 May 1999, by Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico, United States.[3] It is also a Mercury-crosser and the closest known binary system to the Sun with a perihelion of just 0.2 AU.

Orbit[]

The asteroid orbits the Sun at a distance of 0.2–1.1 AU once every 6.18 months (188 days). Its orbit has an eccentricity of 0.69 and an inclination of 39° with respect to the ecliptic.[2] A first precovery was taken by 2MASS at the Fred Lawrence Whipple Observatory in 1998, extending the body's observation arc by one year prior to its official discovery observation at Socorro.[3]

As a potentially hazardous asteroid, it has an Earth minimum orbital intersection distance of 0.0138 AU (2,060,000 km) which corresponds to 5.4 lunar distances.[2] On 25 May 2036, it will pass 0.0155 AU (2,320,000 km) from Earth.[9]

Numbering and naming[]

This minor planet was numbered by the Minor Planet Center on 10 September 2003. It was named from Mohegan legend, after Moshup, a giant who lived in the coastal areas of New England. The asteroid's companion is named Squannit, after the wife of Moshup and a medicine woman of the Makiawisug (little people). The official naming citation was published by the Minor Planet Center on 27 August 2019 (M.P.C. 115894).[10]

Physical characteristics[]

In the SMASS classification, the asteroid a characterized as a stony S-type asteroid.[2]

Satellite[]

Simulated animation of the Moshup binary system

Moshup has a minor-planet moon orbiting it. The moon, named Squannit and designated S/2001 (66391) 1, is approximately 360 metres in diameter, and orbits its primary in every 16 hours at a mean-distance of 2.6 kilometers. The presence of a companion was suggested by photometric observations made by Pravec and Šarounová and was confirmed by radar observations from Arecibo observations and announced on 23 May 2001 (also see below).[5][8]

Diameter and shape[]

Radar images of Moshup taken at Goldstone

According to radiometric observations from Arecibo Observatory, the asteroid has a mean diameter of 1.317 kilometers.[4] The observations were taken from May 21–23, 2001, by Lance A. M. Benner, Steven J. Ostro, Jon D. Giorgini, Raymond F. Jurgens, Jean-Luc Margot and Michael C. Nolan.[4]

The Collaborative Asteroid Lightcurve Link adopts a diameter of 1.3 kilometers and derives an albedo 0.26 with an absolute magnitude of 16.5.[7]

The shapes of the two bodies and their dynamics are complex.[11] With a dimension of 1.5 x 1.5 x 1.34 kilometers for a simple triaxial ellipsoid, the asteroid has an oblate shape, which is dominated by an equatorial ridge at the body's potential-energy minimum. This bizarre property of the equatorial region means that it is close to breakup: raising a particle a meter above the surface would put it into orbit. As seen in the image at above right, the gravitational effects between the moon and the asteroid create a gigantic mountain extending in the equatorial plane around the entire asteroid. It was the first asteroid to be described as "muffin-shaped",[12] which is now understood to be a very common shape for asteroids in critical rotation,[13] including 101955 Bennu and 162173 Ryugu.

Lightcurves[]

During 19–27 June 2000, a rotational lightcurve of this asteroid was obtained from photometric observations by Petr Pravec and Lenka Šarounová at Ondřejov Observatory. Lightcurve analysis gave a rotation period of 2.7650 hours with a brightness variation of 0.12 magnitude (U=3).[5]

In September 2016, the most recent and poorly determined rotational lightcurve with a period of 9.581±0.019 hours was obtained by the Spanish amateur astronomer group OBAS (U=1).[6]

See also[]

References[]

  1. ^ "ESO contributes to protecting Earth from dangerous asteroids". European Southern Observatory. 3 June 2019. Retrieved 3 June 2019.
  2. ^ a b c d e f g h "JPL Small-Body Database Browser: 66391 (1999 KW4)" (2017-05-31 last obs.). Jet Propulsion Laboratory. Retrieved 1 June 2017.
  3. ^ a b c "66391 (1999 KW4)". Minor Planet Center. Retrieved 30 March 2017.
  4. ^ a b c d e Ostro, Steven. J.; Margot, Jean-Luc; Benner, Lance A. M.; Giorgini, Jon D.; Scheeres, Daniel J.; Fahnestock, Eugene G.; et al. (November 2006). "Radar Imaging of Binary Near-Earth Asteroid (66391) 1999 KW4". Science. 314 (5803): 1276–1280. Bibcode:2006Sci...314.1276O. doi:10.1126/science.1133622. Retrieved 1 June 2017.
  5. ^ a b c Pravec, P.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Mottola, S.; Hahn, G.; et al. (March 2006). "Photometric survey of binary near-Earth asteroids". Icarus. 181 (1): 63–93. Bibcode:2006Icar..181...63P. doi:10.1016/j.icarus.2005.10.014. Retrieved 1 June 2017.
  6. ^ a b Lozano, Juan; Flores, Angel; Mas, Vicente; Fornas, Gonzalo; Rodrigo, Onofre; Brines, Pedro; et al. (April 2017). "Seven Near-Earth Asteroids at Asteroids Observers (OBAS) - MPPD: 2016 June-November". The Minor Planet Bulletin. 44 (2): 108–111. Bibcode:2017MPBu...44..108L. ISSN 1052-8091. Retrieved 1 June 2017.
  7. ^ a b c d "LCDB Data for (66391)". Asteroid Lightcurve Database (LCDB). Retrieved 1 June 2017.
  8. ^ a b Johnston, Robert (20 September 2014). "(66391) 1999 KW4". Johnston's Archive. Retrieved 30 March 2017.
  9. ^ "JPL Close-Approach Data: 66391 (1999 KW4)" (2013-05-09 last obs (arc=14.9 yr)). Retrieved 6 April 2016.
  10. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 February 2018.
  11. ^ NASA Jet Propulsion Laboratory Asteroid Radar Research, retrieved May 3, 2007
  12. ^ CBS News - Scientist: Asteroid To Return In 2036,
  13. ^ Jewitt, David; Weaver, Harold; Mutchler, Max; Li, Jing; Agarwal, Jessica; Larson, Stephen (2018). "The Nucleus of Active Asteroid 311P/(2013 P5) PANSTARRS". The Astronomical Journal. 155 (6): 231. arXiv:1804.05897. doi:10.3847/1538-3881/aabdee. ISSN 1538-3881.

External links[]