(8035) 1992 TB

(8035) 1992 TB is an Apollo asteroid, a type of Near-Earth Object. It is also a Venus-crosser and a Mars-crosser, although it doesn't make close approaches to Mars.[5]

(8035) 1992 TB
Orbit of (8035) 1992 TB
Discovery[1]
Discovered bySpacewatch
Discovery siteKitt Peak Observatory
Discovery date2 October 1992
Designations
None
Orbital characteristics[1][2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc8363 days (22.90 yr)
Aphelion1.9625 AU (293.59 Gm)
Perihelion0.72149 AU (107.933 Gm)
1.3420 AU (200.76 Gm)
Eccentricity0.46238
1.55 yr (567.83 d)
145.13°
0° 38m 2.364s / day
Inclination28.308°
185.64°
6.0430°
Earth MOID0.273002 AU (40.8405 Gm)
Jupiter MOID2.99532 AU (448.093 Gm)
Proper orbital elements
0.5068[3]
24.45°[3]
231.32 deg / yr
1.55629 yr
(568.433 d)
Physical characteristics
Dimensions1.673 km (1.040 mi).[4][lower-alpha 1]
17.1

    Encounters with Venus and Earth

    1992 TB makes close approaches to Earth, but often comes many times closer to Venus. Soon after the discovery of the asteroid in 1992, a close approaches of Earth was made. Three years after it was discovered, 1992 TB came 45,720,000 km (0.3056 AU) from Earth.[1] In 2003, (8035) 1992 TB was listed as a potentially hazardous object,[6] but has since been removed. However, 1992 TB is not expected to come within 37,000,000 km (0.25 AU) of Earth in the near future.[1] On the other hand, 1992 TB can come much closer to Venus. Its next Venus encounter was in 29 May 2015, where it came 11,710,000 km (0.0783 AU) from the planet.[5] Its closest approach in the near future will be 7,380,000 km (0.0493 AU).[1]

    Notes
    1. Assuming an albedo of 0.1

    References
    1. "(8035) 1992 TB". JPL Small-Body Database. Jet Propulsion Laboratory. SPK-ID: 2008035. Retrieved 4 April 2016.
    2. "Comets and Asteroids: 8035 (1992 TB)". Find the Data. 11 November 2013. Retrieved 21 November 2013.
    3. "(8035) 1992TB". Neodys. University of Pisa. Retrieved 23 November 2015.
    4. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Sephen F. Austin State University. Dan Burton. Archived from the original on 23 March 2010. Retrieved 26 November 2013.
    5. "Upcoming Close Approaches (< 0.10 AU) of NEOs to the Inner Planets". Shaw. Retrieved 19 November 2013.
    6. "MPEC 2003-V26 : PHAS (2003 NOV. 27.0 TT)". International Astronomical Union. Minor Planet Center. 27 November 2003. Retrieved 21 November 2013.
    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.