3133 Sendai

3133 Sendai
Discovery [1]
Discovered by A. Kopff
Discovery site Heidelberg Obs.
Discovery date 4 October 1907
Designations
MPC designation 3133 Sendai
Named after
 Sendai (Japanese city)[2]
A907 TC · 1968 TO
1973 DN · 1981 UX
1984 QG1 · A907 XA
main-belt · Flora [3]
Orbital characteristics [1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 108.50 yr (39,631 days)
Aphelion 2.5314 AU
Perihelion 1.8298 AU
2.1806 AU
Eccentricity 0.1608
3.22 yr (1,176 days)
282.14°
0° 18m 21.6s / day
Inclination 6.5664°
37.161°
358.31°
Physical characteristics
Dimensions 8.323±0.066 km[4]
7.25±0.30 km[5]
7.47 km (calculated)[3]
5.776±0.005 h[lower-alpha 1]
5.7491±0.0008 h[6]
0.2131±0.0373[4]
0.307±0.039[5]
0.24 (assumed)[3]
S [3]
12.8[1][3]
12.7[4]
12.7[5]
12.522±0.001 (R)[6]
12.92±0.21[7]

    3133 Sendai, provisional designation A907 TC, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered by German astronomer August Kopff at Heidelberg Observatory, southern Germany, on 4 October 1907.[8]

    The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.8–2.5 AU once every 3 years and 3 months (1,176 days). Its orbit has an eccentricity of 0.16 and an inclination of 7° with respect to the ecliptic.[1]

    According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer and its extended NEOWISE mission, the asteroid's surface has an albedo of 0.21 and 0.31, with a diameter of 8.3 and 7.3 kilometers, respectively.[4][5] The Collaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – which derives from 8 Flora, the largest member and namesake of this orbital family – and calculates a concurring diameter of 7.5 kilometers.[3] In 2010, two rotational light-curves were obtained by amateur astronomer Ralph Megna at Goat Mountain Astronomical Research Station (G79), and by the U.S. Palomar Transient Factory in California. The concurring light-curves showed a rotation period of 5.776±0.005 and 5.7491±0.0008 hours, respectively (U=3-/2).[lower-alpha 1][6]

    The minor planet is named for the second largest city north of Tokyo, Sendai (pop. 1 million), location of the Tōhoku University. It is the home of the Sendai Astronomical Observatory, which was founded in 1955, on appeal by the Sendai Amateur Astronomical Association. The observatory has discovered several minor planets.[2] Naming citation was published on 29 September 1985 (M.P.C. 10045).[9]

    References

    1. 1 2 Megna (2011) web: rotation period 5.776±0.005 hours with a brightness amplitude of 0.19 mag. Light-curve chart at Ralph Megna's website and summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (3133) Sendai.
    1. 1 2 3 4 "JPL Small-Body Database Browser: 3133 Sendai (A907 TC)" (2016-04-05 last obs.). Jet Propulsion Laboratory. Retrieved April 2016.
    2. 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (3133) Sendai. Springer Berlin Heidelberg. p. 259. ISBN 978-3-540-00238-3. Retrieved April 2016.
    3. 1 2 3 4 5 6 "LCDB Data for (3133) Sendai". Asteroid Lightcurve Database (LCDB). Retrieved April 2016.
    4. 1 2 3 4 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 April 2016.
    5. 1 2 3 4 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. Retrieved January 2016.
    6. 1 2 3 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 April 2016.
    7. ↑ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved April 2016.
    8. ↑ "3133 Sendai (A907 TC)". Minor Planet Center. Retrieved April 2016.
    9. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved April 2016.

    External links


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