Movatterモバイル変換
[0]ホーム
Asteroids with Satellites Database--Johnston's Archive
(1333) Cevenola
compiled by Wm. Robert Johnston
last updated29 May 2019--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
orbital data, primary (osculating elements)[JPL]: | semimajor axisa: | 2.632135918 AU | | orbital periodP: | 4.270420778 yr
(= 1559.771189 d) | | eccentricitye: | 0.13402285 | | perihelion distanceq: | 2.27936956 AU | | aphelion distanceQ: | 2.984902276 AU | | inclinationi: | 14.64508658° | | argument of perihelionω: | 336.5102622° | | ascending nodeΩ: | 115.1180112° | | mean anomalyM: | 332.7561903° | | perihelion passageTP: | 2014 Sep 18.0391 | | Epoch: | 2014 May 23 | | data arc: | 1934-2013(1041 obs.) | | Earth MOID: | 1.30218 AU | | Jupiter Tisserand invariantTJ: | 3.341 |
orbital data, secondary: | semimajor axisas: | ? | | orbital periodPs: | ? | | eccentricityes: | ? | | normalized ang. mom.αL: | ? |
| other data, system (combined):| absolute mag.H: | 11.4[MPC] | | slope parameterG: | (0.15) [*A] | | effective diameterdE: | 17.15± 0.24 km [M11b] | | geometric albedo: | 0.166± 0.038[M11b] | | color indexU-B: | ? | | color indexB-V: | ? | | taxonomic type: | ? | | massm: | ? | | densityρ: | (1.6 g/cm3) [*A] | | Hill radiusrH: | 2900 km [*E] |
other data, primary: | diameterdp: | 16.2 km [*D] | | rotation periodRPp: | 4.88± 0.02h [W02a] | | amplitude in mag., rotationalΔM: | 0.97± 0.03 [W02a] | | pole directionΒ, λ: | ?,? |
other data, secondary: | diameterds: | 5.67km [*D] | | diameter ratiods/dp: | 0.35 [M09a] | | component mag. differenceΔM: | 2.3 [*D] | | rotation periodRPs: | ? | |
|
--(1333) Cevenola --discovery and notes:
Primary discovered1934 Feb 20from Algiers, Algeriaby O. Bancilhon.Alternate designation(s):1934 DA, 1951 EX.Permanent number assigned -.
Named - for the Cevennes mountains, France.
Companion discovered-usinglightcurve observations.Announced2008 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 SocietySpectral properties of (854) Frostia, (1333) Cevenola and (3623) Chaplin
- Warner, Brian D. 2011, Minor Planet BulletinUpon 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 SocietySpectral Investigation of Binary Asteroids
- Warner, B. D. 2002, Minor Planet BulletinAsteroid Photometry at the Palmer Divide Observatory: Results for 1333 Cevenola and 2460 Mitlincoln
©2008-2014, 2019by Wm. Robert Johnston.
Last modified29 May 2019.Return toHome. Return toAstronomy and Space. Return toAsteroids with Satellites.
[8]ページ先頭