![]() Hubble Space Telescope image of Rumina taken in 2008 | |
Discovery [1] | |
---|---|
Discovered by | A. C. Becker A. W. Puckett J. M. Kubica |
Discovery site | Apache Point Obs. |
Discovery date | 9 September 2005 |
Designations | |
(145451) Rumina | |
Pronunciation | /ruːˈmaɪnə/ |
Named after | Rumīna |
2005 RM43 | |
SDO [2] | |
Orbital characteristics [1] | |
Epoch 2025 May 05 (JD 2460800.5) | |
Uncertainty parameter 1 | |
Observation arc | 48.18 yr (17,596 d) |
Earliest precovery date | 17 November 1976 |
Aphelion | 149.67 AU (22.390 Tm) |
Perihelion | 35.147 AU (5.2579 Tm) |
92.41 AU (13.824 Tm) | |
Eccentricity | 0.6197 |
888.36 yr (324475±19 d) | |
8.226° | |
0° 0m 3.994s / day | |
Inclination | 28.6976° |
84.629° | |
318.672° | |
Physical characteristics | |
≈644 km(derived from occultation; 455 and 460 km measured) [3] 524+96 −103 km [4] | |
Mean density | >0.56 g/cm3 [2] |
6.71 h (0.280 d) | |
0.102 [4] | |
V–R=0.33±0.02 (neutral) [4] B0−V0=0.590 [5] B-R=0.99 [2] | |
20.4 [6] | |
4.52±0.01 [4] 4.4 [1] ·4.8 [7] | |
145451 Rumina (provisional designation 2005 RM43) is a large trans-Neptunian object that resides in the scattered disc region beyond the Kuiper belt. It was discovered on 9 September 2005, by American astronomers Andrew Becker, Andrew Puckett and Jeremy Kubica at Apache Point Observatory in Sunspot, New Mexico. It measures approximately 600 kilometers in diameter.
Rumina has been observed 548 times, with precovery images dating back to 1976. [1] [9] The orbit is well determined with an uncertainty parameter of 1. [1]
In 2018, two stellar occultations by Rumina were observed on 3 February and 24 December. [3] The February occultation yielded a single chord length of 456 km (283 mi). [10] Observations of the December occultation yielded two positive chords, which together suggest an approximate diameter of 644 km (400 mi). [11]
Rumina was named on 1 September 2025, after the Roman goddess Rumīna. [12]
Rumina is a minor Roman goddess who was invoked as a protector of nursing mothers.