2015 TB145

Last updated

2015 TB145
Skull2015-TB145.jpg
Radar image of 2015 TB145 taken by the Arecibo Observatory on 30 October 2015.
Discovery [1]
Discovered by Pan-STARRS
Discovery date10 October 2015
Designations
2015 TB145
Orbital characteristics [2]
Epoch 31 May 2020 (JD  2459000.5)
Uncertainty parameter 0
Observation arc 3.11  yr (1,137 d)
Aphelion 3.9073  AU
Perihelion 0.2941 AU
2.1007 AU
Eccentricity 0.86002
3.04 yr (1,112.1 d)
121.744°
0° 19m 25.364s / day
Inclination 39.6899°
37.698°
121.744°
Earth  MOID 0.00295731 AU (442,407 km)
Jupiter  MOID 2.41052 AU
TJupiter 2.97
Physical characteristics
Dimensions
  • 650±30 m (2130±100 ft) [3]
  • 600 m [4] [5]
0.06 [5]
20.0 [2] [6]

    2015 TB145 is a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 650 meters (2,000 feet) in diameter. [3] It safely passed 1.27 lunar distances from Earth on 31 October 2015 at 17:01 UTC, [7] and passed by Earth again in November 2018.

    Contents

    Discovery

    Discovery image of 2015 TB145 from the Pan-STARRS1 telescope, operated by the Institute for Astronomy at the University of Hawaii. 2015 TB145 discovery.gif
    Discovery image of 2015 TB145 from the Pan-STARRS1 telescope, operated by the Institute for Astronomy at the University of Hawaii.

    The asteroid was first observed on 10 October 2015 by Pan-STARRS at an apparent magnitude of 20 using a 1.8-meter (71 in) Ritchey–Chrétien telescope. [1] [6] [lower-alpha 1] The asteroid was not discovered sooner because it spends most of its time beyond the orbit of Mars, has a large orbital inclination, and is usually well below the plane of the ecliptic. [9] The asteroid last passed within 0.064  AU (9,600,000  km ; 5,900,000  mi ) of Earth on 29 October 1923 and will not pass that close again until 1 November 2088. [7]

    The media has nicknamed the asteroid the "Great Pumpkin" [10] after the animated Halloween television special It's the Great Pumpkin, Charlie Brown , [11] "Spooky", [12] the "Halloween Asteroid", [13] [14] and the "Skull Asteroid" [11] due to its skull-like appearance following radio frequency images taken at Arecibo Observatory and closest approach coincidentally occurring on Halloween day. [11]

    2015 flyby

    2015 TB145 passed 1.27 LD from the earth, and 0.75 LD from the moon. 2015 TB145 flyby.png
    2015 TB145 passed 1.27 LD from the earth, and 0.75 LD from the moon.

    On 31 October 2015 the asteroid passed 0.00191  AU (286,000  km ; 178,000  mi ) from the Moon and then passed 0.00325 AU (486,000 km; 302,000 mi) from Earth. [7]

    The last approach this close by an object with absolute magnitude brighter than 20 was 2004 XP14 on 3 July 2006 at 1.1 lunar distances. The next object this large known to pass this close to Earth is (137108) 1999 AN10 that will pass about 1 lunar distance from Earth on 7 August 2027. [15] It is estimated that there are about 2400 near-Earth asteroids 300–500 meters in diameter, of which about 1100 have been discovered. [16]

    During closest approach to Earth the asteroid reached about apparent magnitude 10, [17] which is much too faint to be seen by the naked eye. Even at peak brightness, the asteroid was a challenging target for amateur astronomers with small telescopes, best seen in the Northern hemisphere. The glare from an 80% waning gibbous Moon also hindered observations.[ citation needed ]

    At 11:00 UT the asteroid was in the constellation of Taurus about 9 degrees from the Moon and moving at a rate of 3.4 degrees per hour. [17] At the time of closest approach of 17:00 UT the asteroid was in the constellation of Ursa Major about 56 degrees from the Moon and moving at a rate of 14.7 degrees per hour. [17] After closest approach it quickly became too faint and too close to the Sun in the sky to be seen. [15]

    2015 TB145 skypath.png

    History of close approaches of large near-Earth objects since 1908(A)
    PHA DateApproach distance in lunar distances Abs. mag
    ( H )
    Diameter(C)
    (m)
    Ref(D)
    Nominal(B)MinimumMaximum
    (152680) 1998 KJ9 1914-12-310.6060.6040.60819.4279–900 data
    (458732) 2011 MD5 1918-09-170.9110.9090.91317.9556–1795 data
    (163132) 2002 CU11 1925-08-300.9030.9010.90518.5443–477 data
    69230 Hermes 1937-10-301.9261.9261.92717.5700-900 [18] data
    69230 Hermes1942-04-261.6511.6511.65117.5700-900 [18] data
    2017 NM6 1959-07-121.891.8461.93418.8580–1300 data
    (27002) 1998 DV9 1975-01-311.7621.7611.76218.1507–1637 data
    2002 NY40 2002-08-181.3711.3711.37119.0335–1082 data
    2004 XP14 2006-07-031.1251.1251.12519.3292–942 data
    2015 TB145 2015-10-311.2661.2661.26620.0620-690 data
    (137108) 1999 AN10 2027-08-071.0141.0101.01917.9556–1793 data
    (153814) 2001 WN5 2028-06-260.6470.6470.64718.2921–943 data
    99942 Apophis 2029-04-130.09810.09630.100019.7310–340 data
    2017 MB1 2072-07-261.2161.2152.75918.8367–1186 data
    2011 SM68 2072-10-171.8751.8651.88619.6254–820 data
    (163132) 2002 CU112080-08-311.6551.6541.65618.5443–477 data
    (416801) 1998 MZ 2116-11-261.0681.0681.06919.2305–986 data
    (153201) 2000 WO107 2140-12-010.6340.6310.63719.3427–593 data
    (276033) 2002 AJ129 2172-02-081.7831.7751.79218.7385–1242 data
    (290772) 2005 VC 2198-05-051.9511.7912.13417.6638–2061 data
    (A) This list includes near-Earth approaches of less than 2 lunar distances (LD) of objects with H brighter than 20.
    (B) Nominal geocentric distance from the center of Earth to the center of the object (Earth has a radius of approximately 6,400 km).
    (C) Diameter: estimated, theoretical mean-diameter based on H and albedo range between X and Y.
    (D) Reference: data source from the JPL SBDB, with AU converted into LD (1 AU≈390 LD)
    (E) Color codes:   unobserved at close approach  observed during close approach  upcoming approaches

    2018 flyby

    Orbit of 2015 TB145 2015 TB145 orbit 2015.png
    Orbit of 2015 TB145

    After it had been unobservable for almost three years, 2015 TB145 was recovered on 7 October 2018 by L. Buzzi at Schiaparelli Observatory (observatory code 204), at apparent magnitude 21. [19]

    The 11 November 2018 flyby was about 0.267  AU (39,900,000  km ; 24,800,000  mi ) from Earth. [7] [20]

    Observations

    Radar imagery

    The close approach was studied with radar using Goldstone, the Green Bank Telescope, [15] and the Arecibo Observatory. It was one of the best radar targets of the year with a resolution as high as 2 meters (7 ft) per pixel. [15] Bistatic radar images created with the Green Bank Telescope had a resolution of 4 meters (13 ft) per pixel. [21] Arecibo images had a resolution of 7.5 meters (25 ft) per pixel. [5]

    30 October31 October
    12:55–13:08 UTC
    1 November
    PIA20041-Asteroid-2015TB145-Animation-20151030.gif Halloween asteroid rotation animation.gif

    Possible cometary origin

    The high orbital inclination and eccentricity suggest 2015 TB145 may be an extinct comet that has shed its volatiles after numerous passes around the Sun. [5] [22] Orbital calculations by Petrus Jenniskens and Jérémie Vaubaillon showed that it was not expected to produce associated meteors in 2015. [23] Any meteoroids were expected to pass more than 0.0007 AU (100,000 km; 65,000 mi) from Earth's orbit. [23]

    If meteoroids related to this asteroid were to cross Earth's path, the radiant is expected to be near Northern Eridanus. [23] Cameras for Allsky Meteor Surveillance (CAMS) did not detect any activity in the presumed area of the sky during 2013 and 2014. [23] The object has a low albedo of 0.06, which is only slightly more than a typical comet that has an albedo of 0.03-0.05. [5]

    Notes

    1. For comparison, around 6 October 2012, the asteroid peaked at about apparent magnitude 20.9, but had a solar elongation of only about 75 degrees while 0.4  AU from Earth. [8]

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