483P/PanSTARRS

483P/PanSTARRS
Canada-France-Hawaii Telescope image of split asteroid pair P/2016 J1 on 6 May 2016, showing comet-like tails on both components
Discovery
Discovered byPan-STARRS 1
Discovery siteHaleakalā Observatory
Discovery date5 May 2016
Designations
P/2016 J1 (PanSTARRS)
Orbital characteristics (fragment A)
Epoch21 June 2016
(JD 2457560.5)
Observation arc153 days (A)
140 days (B)
Earliest precovery date4 March 2016
Orbit typemain-belt (outer· Encke-type · periodic
Aphelion3.896 AU
Perihelion2.448 AU
Semi-major axis3.172 AU
Eccentricity0.2283
Orbital period5.65 yr (2,064 days)
Inclination14.330°
199.856°
Argument of
periapsis
46.585°
Last perihelion24 June 2016
TJupiter3.113
Earth MOID1.461 AU
Jupiter MOID1.227 AU
Physical characteristics
Mean diameter
<0.62+0.18
−0.10
 km
(A)
<0.34+0.12
−0.06
 m
(B)
0.04 (assumed)
C/G
B–V = 0.74±0.04 (A)
B–V = 0.74±0.12 (B)
V–R = 0.36±0.04 (A)
V–R = 0.39±0.12 (B)
Comet total
magnitude
(M1)
16.4±0.4 (A)
17.3±0.8 (B)
Comet nuclear
magnitude (M2)
>19.95+0.18
−0.16
(A)
>21.26+0.23
−0.26
(B)

483P/PanSTARRS (provisional designation P/2016 J1) is a pair of active main-belt asteroids that split apart from each other in early 2010. The brighter and larger component of the pair, P/2016 J1-A, was discovered first by the Pan-STARRS 1 survey at Haleakalā Observatory on 5 May 2016. Follow-up observations by the Canada-France-Hawaii Telescope at Mauna Kea Observatory discovered the second component, P/2016 J1-B, on 6 May 2016. Both asteroids are smaller than 1 kilometre (0.62 mi) in diameter, with P/2016 J1-A being roughly 0.6 km (0.37 mi) in diameter and P/2016 J1-B being roughly 0.3 km (0.19 mi) in diameter. The two components recurrently exhibit cometary activity as they approach the Sun near perihelion, suggesting that their activity is driven by sublimation of volatile compounds such as water.