2014 FE72 is a trans-Neptunian object first observed on 26 March 2014, at Cerro Tololo Inter-American Observatory in La Serena, Chile. It is a possible...
9 KB (515 words) - 22:37, 23 January 2024
Sedna is about 500 AU. In an extreme case, the scattered-disc object 2014 FE72 has a semi-major axis around 1,400 AU, though its distance from the Sun...
27 KB (2,375 words) - 23:06, 18 September 2024
it would be safe from gravitational kicks. 2014 SR349, appears to be anti-aligned with Planet Nine. 2014 FE72, an object with an orbit so extreme that it...
30 KB (2,333 words) - 18:22, 14 August 2024
05 ±6000 14.08 MPC · JPL A/2024 D1 3875.88 ±2456 11.45 ±0.52 MPC · JPL 2014 FE72 3559.58 ±220 6.19 MPC · JPL 541132 Leleākūhonua 2713.25 ±360 5.57 ±0.13...
27 KB (1,667 words) - 23:53, 21 September 2024
2012 VP113 (category 2014 in outer space)
(4–1630 AU) 2013 BL76 (8–1870 AU) 2014 FE72 (36–2680 AU) "2012 VP113". Minor Planet Center. Retrieved 14 November 2018. "MPEC 2014-F40 : 2012 VP113". IAU Minor...
18 KB (1,292 words) - 14:02, 19 September 2024
orbital period of any known periodic minor planet, even larger than that of 2014 FE72; it is calculated to reach several thousand AU (Earth-Sun) distances at...
8 KB (593 words) - 21:34, 14 January 2024
heliocentric semi-major axis in the Solar System (larger ones include 2014 FE72, 2012 DR30, and 2005 VX3). 2013 BL76 has a barycentric semi-major axis...
16 KB (817 words) - 20:44, 19 July 2024
November 2005. 2005 VX3 has a barycentric semi-major axis of ~1026 AU. 2014 FE72 and 2012 DR30 have a larger barycentric semi-major axis. The epoch of...
12 KB (717 words) - 01:02, 10 May 2024
semi-major axis of a minor planet not detected out-gassing like a comet. (2014 FE72 has a larger heliocentric semi-major axis.) 2012 DR30 does have a barycentric...
16 KB (857 words) - 04:05, 3 May 2024
(671088) 2014 FB72 16 Mar 2014 Pan-STARRS 106 Y CEN Y CEN Y R 23.8 0.3 17 15.6 32 4.06 (U:1) catalog · MPC · JPL 2014 FE72 26 Mar 2014 Cerro Tololo Obs. 227...
346 KB (787 words) - 11:19, 8 July 2024