Asteroids with Satellites Database--Johnston's Archive

2013 RJ124

compiled by Wm. Robert Johnston
last updated 15 April 2023

--Orbital and physical data--

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

dynamical type, primary: TNO, Cubewano


orbital data, primary (osculating elements) [JPL] :
semimajor axis a: 44.2268 AU
orbital period P: 294.128 yr
(= 107430 d)
eccentricity e: 0.05743
perihelion distance q: 41.687 AU
aphelion distance Q: 46.7669 AU
inclination i: 4.044879°
argument of perihelion ω: 163.29°
ascending node Ω: 111.078°
mean anomaly M: 107.8°
perihelion passage TP: 1935 Jan 28
Epoch: 2023 Feb 25
data arc: 2013-2020 (32 obs.)
Earth MOID: 40.67 AU
Jupiter Tisserand invariant TJ: 5.924
Neptune Tisserand invariant TN:3.095 [*D]


orbital data, secondary:
semimajor axis as: 34900 ± 5300 km [B23i]
separation/primary radius as/rp:400 [*E]
separation/Hill radius as/rH:0.086 [*E]
orbital period Ps: 1850 ± 270 d [B23i]
eccentricity es: 0.14 ± 0.11 [B23i]
inclination is:90° ± 14.5° [B23i]
ascending node Ωs:103° ± 44.5° [B23i]
argument of pericenter ωs:152° ± 103° [B23i]
mean anomaly M:38° ± 73° [B23i]
Epoch:2013 Sep 10.355
normalized ang. mom. αL: ?

other data, system (combined):
absolute mag. H: 6.38 [MPC]
slope parameter G: (0.15) [*A]
effective diameter dE: 175 km [*E]
geometric albedo: (0.16 ) [*A]
color index U-B: ?
color index B-V: ?
taxonomic type: ?
mass m: 1x1018 ± 2.5x1017 kg [B23i]
density ρ: (0.5 g/cm3) [*A]
Hill radius rH: 410000 km [*E]

other data, primary:
diameter dp: 175 km [*E]
rotation period RPp: ?
amplitude in mag., rotational ΔM: ?
pole direction Β, λ: ? , ?


other data, secondary:
diameter ds: ?
diameter ratio ds/dp: ?
component mag. difference ΔM: ?
rotation period RPs: ?

-- 2013 RJ124 --discovery and notes:

Primary discovered 2013 Sep 10 from Cerro Tololo Observatory, La Serena, Chile by ?.

Companion discovered 2013 Sep 10 by P. H. Bernardinelli et al. using observations from Cerro Tololo Inter-American Observatory, La Serena, Chile. Announced 2023 Apr 06 [B23i].

--Links, more technical:

--Links, less technical:

--Links to ADS abstracts:


© 2023 by Wm. Robert Johnston.
Last modified 15 April 2023.
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