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19741 Callahan

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Main-belt asteroid

19741 Callahan
Discovery
Discovered byLINEAR
Discovery siteLincoln Lab ETS
Discovery date5 January 2000
Designations
MPC designation(19741) Callahan
Named afterDiane Callahan
(mentor at DCYSC)
Alternative designations2000 AN141 · 1978 RQ8
Minor planet categorymain-belt · (inner)
background
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.66 yr (14,121 days)
Aphelion2.5407 AU
Perihelion1.9559 AU
Semi-major axis2.2483 AU
Eccentricity0.1301
Orbital period (sidereal)3.37 yr (1,231 days)
Mean anomaly163.76°
Mean motion0° 17 32.64 / day
Inclination8.0506°
Longitude of ascending node167.39°
Argument of perihelion227.28°
Physical characteristics
Dimensions3.12 km (calculated)
3.876±0.166 km
Synodic rotation period7.2684±0.0015 h
Geometric albedo0.20 (assumed)
0.224±0.044
Spectral typeS
Absolute magnitude (H)14.3 · 14.4 · 14.444±0.004 · 14.89

19741 Callahan (provisional designation 2000 AN141) is a stony background asteroid from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter.

It was discovered on 5 January 2000, by the Lincoln Near-Earth Asteroid Research, LINEAR, at the Lincoln Laboratory's Experimental Test Site, Socorro, New Mexico, and named after a mentor of the 2003 Discovery Channel Young Scientist Challenge.

Orbit and classification

The S-type asteroid orbits the Sun in the inner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,231 days). Its orbit has an eccentricity of 0.13 and an inclination of 8° with respect to the ecliptic. Callahan was first identified as 1978 RQ8 at ESO's La Silla Observatory in 1978, which extends the asteroid's observation arc by 22 years prior to its official discovery observation.

Physical characteristics

In December 2009, a rotational lightcurve for this asteroid was obtained from photometric observations at the U.S. Palomar Transient Factory, California. It gave a rotation period of 7.2684±0.0015 hours with a relatively high brightness variation of 0.81 in magnitude (U=2), indicative of a non-spherical shape.

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Callahan measures 3.9 kilometers in diameter and its surface has an albedo of 0.22. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.1 kilometers, with an absolute magnitude of 14.89.

Naming

This minor planet was named after Diane Callahan, teacher at U.S. Fairfield Middle School, Ohio, who mentored a finalist in the 2003 Discovery Channel Youth Science Challenge (DCYSC), a middle school science competition. The approved naming citation was published by the Minor Planet Center on 10 October 2003 (M.P.C. 49772).

References

  1. ^ "JPL Small-Body Database Browser: 19741 Callahan (2000 AN141)" (2017-05-01 last obs.). Jet Propulsion Laboratory. Retrieved 5 July 2017.
  2. ^ Schmadel, Lutz D. (2006). "(19741) Callahan ". Dictionary of Minor Planet Names – (19741) Callahan, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 142. doi:10.1007/978-3-540-34361-5_1597. ISBN 978-3-540-34360-8.
  3. ^ "19741 Callahan (2000 AN141)". Minor Planet Center. Retrieved 22 March 2016.
  4. ^ "LCDB Data for (19741) Callahan". Asteroid Lightcurve Database (LCDB). Retrieved 17 May 2016.
  5. ^ Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 17 May 2016.
  6. ^ Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 3 December 2016.
  7. ^ Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 17 May 2016.
  8. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 17 May 2016.

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