2018 GE3
The orbit of 2018 GE3 with 30-day markers
Discovery [1]
Discovered byCatalina Sky Srvy.
Discovery siteCatalina Stn.
Discovery date14 April 2018
(first observed only)
Designations
2018 GE3
NEO · Apollo [1][2]
Orbital characteristics [2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 7
Observation arc4 days
Aphelion3.3782 AU
Perihelion0.3179 AU
1.8481 AU
Eccentricity0.8280
2.51 yr (918 d)
333.94°
0° 23m 32.28s / day
Inclination8.7368°
25.412°
300.17°
Earth MOID0.0010 AU (0.3896 LD)
Mercury MOID0.0101 AU
Venus MOID0.0556 AU
Mars MOID0.0527 AU
Physical characteristics
Mean diameter
48–110 m[3]
48 m (est. at 0.24)[4]
100 m (est. at 0.05)[4]
23.813[2]

    2018 GE3 is a sub-kilometer asteroid on a highly eccentric orbit, classified as a near-Earth object of the Apollo group, approximately 48–110 meters (160–360 feet) in diameter. It was first observed on 14 April 2018, by astronomers with the Catalina Sky Survey one day prior to its sub-lunar close encounter with Earth at 0.5 lunar distance.[2] It is one of the largest known asteroids (possibly the largest) in observational history to ever pass that close to Earth (also see list).

    Orbit and classification

    2018 GE3 is a member of the near-Earth population of asteroids known as Apollos.[1][2] Apollo asteroids cross the orbit of Earth and are the largest group of near-Earth objects with nearly 10 thousand known members. Based on an observation arc of 4 days, it orbits the Sun at a distance of 0.3–3.4 AU once every 2 years and 6 months (918 days; semi-major axis of 1.85 AU). Its orbit has an unusually high eccentricity of 0.83 and an inclination of 9° with respect to the ecliptic.[2] It is also a Mercury-, Venus- and Mars-crosser, reaching its furthest point from the Sun in the outer asteroid belt. The body's observation arc begins at Steward Observatory's Catalina Station with its first observation in April 2018.[1]

    Close encounters

    In observational history, and other than possibly 2002 MN and 2017 VW13, this asteroid is the largest known object to ever pass that close to Earth, as well as the Moon (also see History of closest approaches of large near-Earth objects).[lower-alpha 1] 99942 Apophis will break both of these records when it approaches only 0.098 LD (0.000252 AU) from Earth on 13 April 2029.

    2018 flyby

    Trajectory past the Earth and Moon
    Magnitude estimates

    2018 GE3 was first observed on 14 April 2018, at 09:23 UT by astronomers at Steward Observatory's Catalina Station, Arizona, the day prior to its close encounter with Earth.

    It had been more than 120 degrees from the Sun since March 2018, but was simply too far and too faint to be detected by automated surveys. Despite coming from directly away from the Sun, it was not discovered until 14 April 2018, only one day prior to its closest approach. If the most advanced survey telescopes had been looking at its location, it could have been discovered as early as 30 March. On 15 April 2018, at 06:41 UT, this object passed Earth at a nominal distance of 0.50 LD (0.001289 AU) which corresponds to a distance of 193,000 kilometres (120,000 miles), at a speed of 29.5 km/s (66,000 mph).[2][3] The object also approached the Moon at an even closer distance of 0.34 LD (0.00087 AU) a few hours later, at 09:59 UT.[2]

    It was the 32nd known asteroid to flyby Earth within 1 lunar distance (LD) since the start of 2018 and 16th closest, although it was the largest known asteroid to pass within half a lunar distance. After closest approach its apparent magnitude dropped from 12 to 35 in less than 12 hours, heading towards the Sun. Coming from the opposite direction, it would have been impossible to observe before its approach. A preliminary analysis of the orbit of 2018 GE3 shows that this is the closest this particular asteroid has come to Earth since at least 1930.[3]

    Animation of 2018 GE3's orbit
    Around the Sun
    Around the Earth
      2018 GE3 ·   Sun ·   Earth ·   Moon

    Historical close encounters

    History of closest approaches of large near-Earth objects since 1914
    (less than H 24 and 1 LD)(A)
    NEO Date Approach distance in lunar distances Abs. mag
    (H)    		 Diameter (C)
    (m)    		 Ref (D)
    Nominal(B) Minimum Maximum
    (152680) 1998 KJ91914-12-310.6060.6040.60819.4279–900data
    (458732) 2011 MD51918-09-170.9110.9090.91317.9556–1795data
    (163132) 2002 CU111925-08-300.9030.9010.90518.5443–477data
    2010 VB11936-01-060.5530.5530.55323.248–156data
    2002 JE91971-04-110.6160.5870.65121.2122–393data
    2013 UG11976-10-170.8540.8530.85522.373–237data
    2012 TY521982-11-040.8180.8130.82221.4111–358data
    2012 UE341991-04-080.8470.6761.02723.346–149data
    2017 VW132001-11-080.3730.3163.23620.7153–494data
    2002 MN2002-06-140.3120.3120.31223.640–130data
    (308635) 2005 YU552011-11-080.8450.8450.84521.9320–400data
    2011 XC22011-12-030.9040.9010.90723.248–156data
    2018 AH2018-01-020.7730.7720.77322.567–216data
    2018 GE32018-04-150.5020.5010.50323.735–135data
    2010 WC92018-05-150.5280.5280.52823.542–136data
    (153814) 2001 WN52028-06-260.6470.6470.64718.2921–943data
    99942 Apophis2029-04-130.09890.09890.098919.7310–340data
    2012 UE342041-04-080.2830.2740.35423.346–149data
    2015 XJ3512047-06-060.7890.25138.13522.470–226data
    2007 TV182058-09-220.9180.9170.91923.837–119data
    2005 WY552065-05-280.8650.8560.87420.7153–494data
    (308635) 2005 YU552075-11-080.5920.4990.75221.9320–400data
    (456938) 2007 YV562101-01-020.6210.6150.62821.0133–431data
    2007 UW12129-10-190.2390.1550.38122.761–197data
    101955 Bennu2135-09-250.5310.5070.55520.19472–512data
    (153201) 2000 WO1072140-12-010.6340.6310.63719.3427–593data
    2009 DO1112146-03-230.8960.7441.28822.858–188data
    (85640) 1998 OX42148-01-220.7710.7700.77121.1127–411data
    2011 LT172156-12-160.9980.9551.21521.6101–327data
    (A) This list includes near-Earth approaches of less than 1 lunar distances (LD) of objects with H brighter than 24.
    (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 0.05 and 0.25.
    (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
    Note: All close approaches between 1900 and 2200 are listed (with H<24 at less than 1 LD). Objects not observed during the approach,
    and simply estimated to have approached on this date, are colored grey. Generically estimated asteroid diameters are given in italics.

    Asteroid 2002 MN passed closer to Earth than 2018 GE3 in 2002, and had a brighter absolute magnitude (H) of 23.6, and could be either larger or smaller than 2018 GE3, depending on their albedos and thus exact sizes. 2017 VW13 (H=20.7) may have also passed closer in 2001, although the distance of its approach is very uncertain and it was not discovered until 2017.[5]

    Physical characteristics

    Diameter and albedo

    The diameter can only be estimated based on the brightness and distance. The albedo is currently unknown. Based on a generic magnitude-to-diameter conversion, 2018 GE3 measures between 48–100 meters (157–328 feet) in diameter, for an absolute magnitude of 23.8,[2] and an assumed albedo between 0.05 and 0.24, which represent typical values for carbonaceous and stony asteroids, respectively.[4]

    This asteroid is about three to six times the diameter of the meteor that exploded in the skies above Chelyabinsk, Russia in February 2013, which damaged over 7,200 buildings and injured 1,500 people, mostly from flying glass. If an asteroid of this size were to enter Earth's atmosphere, a good portion of it would likely disintegrate due to friction with the air. The remnants could survive entry however and impact the surface, thus causing regional damage dependent on various factors such as composition, speed, entry angle, and location of impact.[3]

    Rotation period

    As of 2018, no rotational lightcurve of 2018 GE3 has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[2]

    Numbering and naming

    This minor planet has neither been numbered nor named.[1]

    See also

    Notes

    1. ↑ 2002 MN has a brighter absolute magnitude than this asteroid (23.6 vs. 23.8) and may therefore be larger. Note that the term "observational history" excludes objects such as 2017 VW13 not yet discovered at the time of close approach. Furthermore, 2017 VW13's orbit is uncertain enough that it may not have passed closer than 2018 GE3 at all.

    References

    1. 1 2 3 4 5 "2018 GE3". Minor Planet Center. Retrieved 15 April 2018.
    2. 1 2 3 4 5 6 7 8 9 10 "JPL Small-Body Database Browser: (2018 GE3)" (15 April 2018 last obs.). Jet Propulsion Laboratory. Retrieved 28 April 2018.
    3. 1 2 3 4 "Asteroid buzzed Earth this weekend". EarthSky. Retrieved 16 April 2018.
    4. 1 2 3 "Asteroid Size Estimator". CNEOS NASA/JPL. Retrieved 28 April 2018.
    5. ↑ "JPL Small-Body Database Browser: (2017 VW13)" (4 March 2018 last obs.). Jet Propulsion Laboratory.
    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.