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C / 2015 ER 61 (PANSTARRS)


2015 ER 61 is a comet , a centaur , an internal object of the Oort cloud , one of the comets approaching the Earth , and, possibly, a Damocloid .

2015 ER 61
Dwarf planet
Category of small planetsNear Earth Object , Cupid , Daclmoid , Scattered Disk Object, Centaur
Opening
DiscovererPan-STARRS 1 (F51)
opening dateMarch 15, 2015
Orbital characteristics
Epoch : June 27, 2015 ( JD 2457200.5)
Perihelion1.059306 ± 0.000046 a.e
Aphelion2456 ± 62 a. e.
1425/854 a. e.
Semi-axis ( a )1229 ± 31 a. e.
715/428 a. e. [1]
The eccentricity of the orbit ( e )0.999138 ± 0.000022
Sidereal period of circulation43060 ± 1620 years
(1.6 × 10 7 ± 5.9 × 10 5 days)
Average anomaly ( M o )359.98435 ± 0.00059 °
Inclination ( i )6,129721 ± 0,000071 °
Ascending node longitude ( Ω )238.8124 ± 0.0022 °
Pericenter Argument ( ω )64.0806 ± 0.0020 °
physical characteristics
Dimensions9–22 km [2]
20 km [3]
Albedo~ 0.05 (presumably)
Apparent magnitude14.74 (peak May 1, 2017)
Absolute magnitude12.2

It occupies one of the first places in the largest aphelion among the known minor planets of the Solar System , yielding to such objects as 2014 FE72 , 2005 VX3 , 2009 FW54 (2012 DR30), 2013 SY 99 , (308933) 2006 SQ372 and 2013 BL 76 . In addition, it has the highest eccentricity of the orbit of all known minor planets, the distance to the Sun when moving in its orbit changes by about 99.9%, the next object in 2005 VX 3 has an eccentricity of 0.9973. February 1, 2016 was classified as a comet when it was at a distance of 5.7 a. e. from the Sun [4] .

It is closely converging with Jupiter , which in the past has thrown it into modern long-range orbit.

Content

Perihelion 2017

2015 EP 61 was discovered on March 15, 2015 at a distance of 8.44 a. e. from the Sun and had a magnitude 21.5 m . In September 2015, its magnitude was 21.2 m and slowly increased. At the beginning of February 2016, the comet reached a stellar magnitude of 20 m and on March 28, 2016 it will approach Jupiter by 0.9245 A. e. This will lead to a change in its orbit, significantly reducing its aphelion from 1430 a. E. ~ 1200 a. e. When passing through the inner part of the Solar system, the aphelion will first decrease to 160 a. e. in the spring of 2017, and then it will increase and by 2020 will be 854 a. e. 

On April 4, 2017, the ER 61 will reach the point of closest approach to Earth ~ 1.42 a. e. At this moment it will reach a stellar magnitude of 14.8 m , and, assuming its size to be 20 km, will have an apparent size of 19 milliseconds of arc.

Comparison

 
2015 ER61 compared to some other celestial bodies with a very distant orbit. Including (90377) Sedna , 2015 DB216 (orbit is specified incorrectly), (87269) 2000 OO67 , VN112 2004 , 2005 VX3 , (308933) 2006 SQ372 , 2007 TG422 , 2007 DA61 , MS9 2009 , 2010 GB174 , 2010 NV1 , 2010 BK118 , 2012 DR30 , 2012 VP113 , 2013 BL76 , 2013 AZ60 , 2013 RF98

Orbital characteristics

Distance to the sun
( A. e. )
EventThe epochAphelion
(Q)
Perihelion
(q)
Big axis
(a)
Eccentricity
(e)
Period
(p)
Mood
(i)
Ascending node longitude
(Ω)
Medium anomaly
(M)
Pericenter argument
(ω)
but. e.(years old)(°)
36.52000/01/011423.41.05378712.20.9985218.9906.12745239.06359.67163.99
20.22010/01/011435.41.05377718.20.9985319,2406.12732239.03359.86264.01
9.012015/01/011430.81.05347715.90.9985319,1406.12819238.97359.95664.08
8.44opening2015/03/151436.11.05313718.60.9985319,2506.12879238.95359.96064.11
6.0082016/01/011667.31.04763834.20.9987424,0806.15827238.25359.98064.92
5.204approach to Jupiter2016/03/281291.91.04030646.50.9983916,4206.24250236.73359.97666.64
2.2422017/01/01324.61.03505162.80.993642,0806.34928235.27359.93968.46
1.079rapprochement with the Earth2017/04/04164.31.0383082.70.987447506.34595235.27359.95368.30
1.0397perihelion2017/05/10210.01.03973105.50.990151,0806.34423235.25000.000467.92
3.4372018/01/011091.11.04449546.10.9980912,7506.34438235.23000.01868.27
9.782020/01/01857.81.04583429.40.997568,8906.34009235.21000.10768.29
56.032050/01/01854.61.04649427.80.997558,8406.33543235.18001.32968.34

Links

  • C / 2015 ER61 in the minor planets database JPL

Notes

  1. ↑ Since the 2015 ER61 orbit is so far away from the Sun, a barycentric solution is a more accurate value for its orbit. In addition, a close approach to Jupiter in 2016, and a journey through the inner solar system in 2017 will drastically change its orbit. Therefore, orbits are provided for 2000–2016 and 2018–2100, respectively.
  2. ↑ Glossary: ​​Absolute Magnitude (H) (English) . JPL . Nasa The appeal date is September 14, 2015.
  3. Assuming an albedo of 0.05, like that of comets
  4. ↑ MPEC 2016-C01: COMET C / 2015 ER61 (PANSTARRS) (Eng.) . IAU Minor Planet Center (1 February 2016). The appeal date is February 1, 2016. (CK15E61R)
Source - https://ru.wikipedia.org/w/index.php?title=C/2015_ER61_(PANSTARRS)&oldid=84747090


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