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Asteroids with Satellites Database--Johnston's Archive

(5426) Sharp

compiled by Wm. Robert Johnston
last updated9 October 2021

--Orbital and physical data--

(Seethis page for definitions of quantities; source codes in brackets, seethis link for full references; *A, *D, and *E indicate assumed, derived, and estimated values, respectively.)

dynamical type, primary:main belt asteroid, inner


orbital data, primary (osculating elements)[JPL]:

semimajor axisa:1.9550247279 AU
orbital periodP:2.733610189 yr
(= 998.4511217 d)
eccentricitye:0.11656562
perihelion distanceq:1.727136059 AU
aphelion distanceQ:2.1829133971 AU
inclinationi:23.79822738°
argument of perihelionω:67.3917973°
ascending nodeΩ:88.1698003°
mean anomalyM:103.0700876°
perihelion passageTP:2020 Sep 18.137654
Epoch:2021 Jul 01
data arc:1985-2021(1958 obs.)
Earth MOID:0.824181 AU
Jupiter Tisserand invariantTJ:3.776

orbital data, secondary:

semimajor axisas:4.4 km[*E]
separation/primary radiusas/rp:4.5 [*E]
separation/Hill radiusas/rH:0.017 [*E]
orbital periodPs:1.0092± 0.0008d [W15j]
eccentricityes:?
normalized ang. mom.αL:?
other data, system (combined):
absolute mag.H:14.06[MPC]
slope parameterG:(0.15) [*A]
effective diameterdE:2.03± 0.34 km [M11b]
geometric albedo:1[M11b]
color indexU-B:?
color indexB-V:?
taxonomic type:?
massm:?
densityρ:(1.6 g/cm3) [*A]
Hill radiusrH:270 km [*E]

other data, primary:

diameterdp:1.97± 0.33 km [*E]
rotation periodRPp:4.5609± 0.0001h [W15j]
amplitude in mag., rotationalΔM:0.18± 0.01 [W15j]
amplitude in mag., mutual eventsΔM:0.08 ±0.01 [W15j]
pole directionΒ, λ:?,?

other data, secondary:

diameterds:>0.49km [*E]
diameter ratiods/dp:>0.25 [*E]
component mag. differenceΔM:<3.01 [*E]
rotation periodRPs:24.22± 0.02h [W15j]

--(5426) Sharp --discovery and notes:

Primary discovered1985 Feb 16from Palomar Observatory, California, USAby C. S. Shoemaker.Alternate designation(s):1985 DD.Permanent number assigned 1993 Feb 06.

Named 1995 Mar 17 for Robert P. Sharp (1911-2004) [MPC024917].

Companion discovered2014 Dec 29 by B. D. Warner, V. Benishek, and A. Ferrerousinglightcurve observations from Palmer Divide Station, Eaton, Colorado, USA; Belgrade Astronomical Observatory, Belgrade, Serbia; Bigmuskie Observatory, Mombercelli, Astri, Italy.Announced2015 Jun [W15j].

--Links, more technical:

--Links, less technical:

--Links to ADS abstracts:


©2015, 2021by Wm. Robert Johnston.
Last modified9 October 2021.
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