Asteroids with Satellites Database--Johnston's Archive
(1333)
Cevenola
compiled by Wm. Robert Johnston
last updated
29 May 2019
--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:
main belt asteroid
orbital data, primary (osculating elements)
[JPL]
: |
semimajor axis a: |
2.632135918 AU
| |
orbital period P: |
4.270420778 yr
(= 1559.771189 d)
| |
eccentricity e: |
0.13402285
| |
perihelion distance q: |
2.27936956 AU
| |
aphelion distance Q: |
2.984902276 AU
| |
inclination i: |
14.64508658°
| |
argument of perihelion ω: |
336.5102622°
| |
ascending node Ω: |
115.1180112°
| |
mean anomaly M: |
332.7561903°
| |
perihelion passage TP: |
2014 Sep 18.0391
| |
Epoch: |
2014 May 23
| |
data arc: |
1934-2013
(1041 obs.)
| |
Earth MOID: |
1.30218 AU
| |
Jupiter Tisserand invariant TJ: |
3.341
|
orbital data, secondary:
|
semimajor axis as: |
?
| |
orbital period Ps: |
?
| |
eccentricity es: |
?
| |
normalized ang. mom. αL: |
?
|
|
other data, system (combined):
|
absolute mag. H: |
11.4
[MPC]
| |
slope parameter G: |
(0.15) [*A]
| |
effective diameter dE: |
17.15
± 0.24
km [M11b]
| |
geometric albedo: |
0.166
± 0.038
[M11b]
| |
color index U-B: |
?
| |
color index B-V: |
?
| |
taxonomic type: |
?
| |
mass m: |
?
| |
density ρ: |
(1.6
g/cm3) [*A]
| |
Hill radius rH: |
2900 km [*E]
|
other data, primary:
|
diameter dp: |
16.2
km [*D]
| |
rotation period RPp: |
4.88
± 0.02
h [W02a]
| |
amplitude in mag., rotational ΔM: |
0.97
± 0.03
[W02a]
| |
pole direction Β, λ: |
?
,
?
|
other data, secondary:
|
diameter ds: |
5.67
km [*D]
| |
diameter ratio ds/dp: |
0.35
[M09a]
| |
component mag. difference ΔM: |
2.3
[*D]
| |
rotation period RPs: |
?
| |
|
|
--
(1333) Cevenola
--discovery and notes:
Primary discovered
1934 Feb 20
from
Algiers, Algeria
by
O. Bancilhon.
Alternate designation(s):
1934 DA,
1951 EX.
Permanent number assigned -.
Named - for the Cevennes mountains, France.
Companion discovered
-
using
lightcurve
observations.
Announced
2008 Oct 12.
--Links, more technical:
--Links, less technical:
--Links to ADS abstracts:
- Birlan, M., Nedelcu, D. A., Descamps, P., Berthier, J., Marchis, F., Merouane, S., & Popescu, M. 2011, Monthly Notices of the Royal Astronomical Society Spectral properties of (854) Frostia, (1333) Cevenola and (3623) Chaplin
- Warner, Brian D. 2011, Minor Planet Bulletin Upon Further Review: VI. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory
- Birlan, Mirel, Nedelcu, D., Descamps, P., Berthier, J., Marchis, F., & Merouane, S. 2008, Bulletin of the American Astronomical Society Spectral Investigation of Binary Asteroids
- Warner, B. D. 2002, Minor Planet Bulletin Asteroid Photometry at the Palmer Divide Observatory: Results for 1333 Cevenola and 2460 Mitlincoln
©
2008-2014, 2019
by Wm. Robert Johnston.
Last modified
29 May 2019.
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