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C/2013 US10 (Catalina)

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(Redirected fromC/2013 US10)
Oort cloud comet

For other comets of the same name, seeList of comets discovered by the Catalina Sky Survey.
C/2013 US10 (Catalina)
C/2013 US10 as seen on 9 Dec 2015. To the upper left is theion gas tail and to the lower right is the dust tail.
Discovery
Discovered byCatalina Sky Survey (703)[1][2]
Discovery date31 October 2013
Orbital characteristics
Epoch4 December 2015[3]
Observation arc4.26 years
Number of
observations
4396
Orbit typeOort cloud
Aphelion~38000AU (inbound)[4]
Perihelion0.8229AU (q)[3]
Eccentricity1.0003[3]
1.000+ (heliocentric epoch 2475–2500)[5]
Orbital periodseveral million years inbound (barycentric solution forepoch 1950)[4]
Ejection trajectory outbound
(barycentric solution for epoch 2050)[4]
Inclination148.87°[3]
Last perihelion15 November 2015[3]
JupiterMOID1.13 AU

C/2013 US10 (Catalina) is anOort cloudcomet discovered on 31 October 2013 by theCatalina Sky Survey at anapparent magnitude of 19 using a 0.68-meter (27 in)Schmidt–Cassegrain telescope.[1] From September 2015 to February 2016 the comet was aroundapparent magnitude 6.[6] The comet took around a million years to complete half an orbit from its furthest distance in the Oort cloud and should be ejected from the Solar System over many millions of years.

Overview

[edit]

When discovered on 31 October 2013 observations from another object from 12 September 2013 were used in the preliminaryorbit determination giving an incorrect solution that suggested anorbital period of only 6 years.[1] But by 6 November 2013 a longerobservation arc from 14 August until 4 November made it apparent that the first solution had the wrong object from 12 September.[2]

By early May 2015 the comet was aroundapparent magnitude 12 and had anelongation of 60 degrees from the Sun as it moved further into theSouthern Hemisphere.[7] The comet came tosolar conjunction on 6 November 2015 when the comet was around magnitude 6.[6] The comet came toperihelion (closest approach to the Sun) on 15 November 2015 at a distance of 0.82 AU from the Sun.[3] At perihelion, it had a velocity of 46.4 km/s (104,000 mph) with respect to the Sun which is slightlygreater than the Sun's escape velocity at that distance. It crossed thecelestial equator on 17 December 2015 becoming aNorthern Hemisphere object. On 17 January 2016 the comet passed 0.72 AU (108,000,000 km; 67,000,000 mi) from Earth and was around magnitude 6[6] while located in theconstellation ofUrsa Major.[8]

C/2013 US10 closest Earth approach on 2016-Jan-17 05:25 UT
Date & time of
closest approach
Earth distance
(AU)
Sun distance
(AU)
Velocity
wrt Earth
(km/s)
Velocity
wrt Sun
(km/s)
Uncertainty
region
(3-sigma)
Reference
2016-01-17 05:250.7247 AU (108.41 million km; 67.37 million mi; 282.0 LD)1.388 AU (207.6 million km; 129.0 million mi; 540 LD)59.035.8± 125 kmHorizons

C/2013 US10 is dynamically new. It came from theOort cloud with a loosely bound chaotic orbit that was easily perturbed bygalactic tides andpassing stars. Before entering the planetary region (epoch 1950),C/2013 US10 had an orbital period of several million years.[4] After leaving the planetary region (epoch 2050), it will be on anejection trajectory.[4] TheSun's escape velocity at 200 AU is 2.98 km/s[9] and the comet will be going 3.0 km/s at 200 AU from the Sun.[10]

C/2013 US10 distance and velocity compared to the Sun with a 400 year stepsize[11]
DateSun distance
(AU)
Velocity
wrt Sun
(km/s)
Uncertainty
region
(3-sigma)
1615-11-15304.0 AU (45.48 billion km; 28.26 billion mi)2.40± 3 million km
Perihelion0.823 AU (123.1 million km; 76.5 million mi)46.4± 140 km
2415-11-15306.9 AU (45.91 billion km; 28.53 billion mi)2.44± 5 million km

Gallery

[edit]
  • Comet C/2013 US10 (Warsaw, Poland; 10 January 2016, 02:51 UT+1)
    CometC/2013 US10 (Warsaw, Poland; 10 January 2016, 02:51 UT+1)
  • C/2013 US10 imaged on 6 December 2015
    C/2013 US10 imaged on 6 December 2015
  • C/2013 US10 imaged on 6 December 2015 (black and white)
    C/2013 US10 imaged on 6 December 2015 (black and white)

References

[edit]
  1. ^abc"MPEC 2013-V05 : 2013 US10".IAU Minor Planet Center. 2 November 2013. Retrieved15 September 2014. (K13U10S)
  2. ^ab"MPEC 2013-V31 : COMET C/2013 US10 (CATALINA)". IAU Minor Planet Center. 6 November 2013. Retrieved15 September 2014. (CK13U10S)
  3. ^abcdef"MPEC 2014-R69 : Observations and Orbits of Comets". IAU Minor Planet Center. 7 September 2014. Retrieved15 September 2014.
  4. ^abcdeHorizons output."Barycentric Osculating Orbital Elements for Comet C/2013 US10 (Catalina)". Solution using the Solar SystemBarycenter. Ephemeris Type:Elements and Center:@0 (To be outside planetary region, inbound epoch 1950 and outbound epoch 2050)
  5. ^Horizons output."Heliocentric Osculating Orbital Elements for Comet C/2013 US10 (Catalina) for 2450–2500". (2482 has EC= 1.0003)
  6. ^abcSeiichi Yoshida (13 September 2014)."C/2013 US10 ( Catalina )". Seiichi Yoshida's Comet Catalog. Retrieved15 September 2013.
  7. ^"Elements and Ephemeris for C/2013 US10 (Catalina)". IAU Minor Planet Center. Archived fromthe original on 17 May 2014. Retrieved15 September 2014.
  8. ^"Horizons Batch for 2016-01-17 Earth Approach".JPL Horizons. Retrieved2 February 2023.
  9. ^"To the Voyagers and escaping from the Sun". Initiative for Interstellar Studies. 25 February 2015. Retrieved3 February 2023.
  10. ^"Horizons Batch for 200 AU".JPL Horizons. Retrieved3 February 2023.
  11. ^"Horizons Batch for Distance and Velocity using a 400 year stepsize".JPL Horizons. Retrieved3 February 2023.

External links

[edit]
Wikimedia Commons has media related toC/2013 US10 (Catalina).
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