1139 Atami

1139 Atami[1]
Discovery
Discovered by Okuro Oikawa and Kazuo Kubokawa
Discovery date 1 December 1929
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 85.69 yr (31297 days)
Aphelion 2.44496706932325 AU (365.76186750237 Gm)
Perihelion 1.4501914936712 AU (216.94555956046 Gm)
1.94757928149723 AU (291.35371353142 Gm)
Eccentricity 0.25538769720514
2.72 yr (992.75 d)
325.8028921925650°
 21m 45.461s / day
Inclination 13.0861259136982°
213.3506333014720°
206.5615422612800°
Known satellites 1[2]
Earth MOID 0.470132 AU (70.3307 Gm)
Jupiter MOID 2.93913 AU (439.688 Gm)
Jupiter Tisserand parameter 3.824
Physical characteristics
Dimensions ~6km[2]
27.446 h (1.1436 d)

S   (Tholen)

S   (SSMASSII)
12.51

    1139 Atami is a Mars-crossing asteroid orbiting the Sun. It makes a revolution around the Sun once every 3 years. It completes one rotation once every 27 hours. It was discovered by Okuro Oikawa and Kazuo Kubokawa on December 1, 1929.[1] It is named after a harbor near Tokyo, Japan. Its provisional designation was 1929 XE.[3]

    Binary system

    Photometric and Arecibo echo spectra observations in 2005 confirmed a 5 km (3 mi) satellite orbiting at least 15 km (9 mi) from the primary.[2] Due to the similar size of the primary and secondary the Minor Planet Center lists this as a binary companion.[4]

    References

    1. 1 2 3 "JPL Small-Body Database Browser: 1139 Atami (1929 XE)". Retrieved 1 May 2016.
    2. 1 2 3 "Electronic Telegram No. 430". IAU Central Bureau for Astronomical Telegrams. 2006-03-14. Retrieved 2011-01-25.
    3. Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names. Springer. ISBN 3-540-00238-3.
    4. "Satellites and Companions of Minor Planets". IAU Central Bureau for Astronomical Telegrams. 2009-09-17. Retrieved 2011-01-25.

    External links

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