483P/PanSTARRS

< 483P

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):18
<0.34+0.12
−0.06
 m
(B):18
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):18
>21.26+0.23
−0.26
(B):18

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 brightest and largest 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.:18 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.