Table 1
TNOs for which candidate stellar occultations for the period from 2012 Jun. 1st to 2014 Dec. 31st were predicted.
RA(J2000)Dec | RA(J2000)Dec | D | Diameter | Source for | |||
Target ID | Type | Easternmost | Westernmost | V | (AU) | (km) | diameter |
|
|||||||
(8405) Asbolus (also 1995 GO) | CEN | 04:16 +37:05 | 03:19 +33:12 | 21.7 | 16.8 | 84 | [1] |
(24835) 1995 SM55 | TNO | 02:55 +30:48 | 02:34 +28:21 | 20.8 | 38.4 | <704 | [1] |
(10199) Chariklo (also 1997 CU26) | CEN | 17:41 −38:31 | 16:07 −39:52 | 18.2 | 14.5 | 248 | [1] |
(26375) 1999 DE9 | TNO | 12:07 −06:01 | 11:40 −02:40 | 20.6 | 37.3 | 461 | [1] |
(47171) 1999 TC36 | TNO | 02:11 +05:02 | 01:44 +02:13 | 19.8 | 30.6 | 393 | [1] |
(38628) Huya (also 2000 EB173) | TNO | 15:53 −06:01 | 15:16 −04:07 | 19.3 | 28.6 | 458 | [1] |
(54598) Bienor (also 2000 QC243) | CEN | 01:54 +30:30 | 00:54 +22:50 | 17.5 | 16.7 | 188 | [1] |
(55565) 2002 AW197 | TNO | 09:42 +00:48 | 09:25 +03:24 | 20.1 | 46.1 | 742 | [1] |
(55576) Amycus (also 2002 GB10) | CEN | 17:50 −33:58 | 16:42 −34:08 | 20.2 | 18.1 | 101 | [1] |
(83982) Crantor (also 2002 GO9) | CEN | 19:41 −19:46 | 18:36 −19:34 | 21.0 | 16.7 | 60 | [1] |
(119951) 2002 KX14 | TNO | 16:48 −22:39 | 16:28 −22:00 | 20.5 | 39.3 | 455 | [1] |
(307261) 2002 MS4 | TNO | 18:29 −07:42 | 18:13 −08:14 | 20.6 | 47.0 | 934 | [1] |
(84522) 2002 TC302 | TNO | 02:20 +25:49 | 02:05 +23:26 | 20.5 | 45.8 | 584 | [1] |
(55637) 2002 UX25 | TNO | 02:36 +10:12 | 02:18 +09:19 | 19.9 | 41.3 | 697 | [1] |
(55638) 2002 VE95 | TNO | 05:31 +08:43 | 04:59 +08:44 | 20.4 | 28.8 | 250 | [1] |
(119979) 2002 WC19 | TNO | 05:31 +19:00 | 05:12 +18:17 | 21.3 | 41.8 | 363 | [2] |
(120132) 2003 FY128 | TNO | 13:14 −15:59 | 12:50 −13:02 | 20.8 | 39.2 | 460 | [1] |
(174567) 2003 MW12 | TNO | 17:09 −02:41 | 17:00 −01:51 | 20.2 | 47.3 | 724 | [2] |
(120178) 2003 OP32 | TNO | 22:11 +02:29 | 21:52 +02:41 | 20.4 | 41.8 | 561 | [2] |
2003 UZ413 | TNO | 03:28 +06:23 | 03:11 +05:25 | 20.7 | 43.0 | 501 | [2] |
(84922) 2003 VS2 | TNO | 04:51 +33:44 | 04:24 +33:35 | 19.8 | 36.5 | 523 | [1] |
(90568) 2004 GV9 | TNO | 14:39 −25:59 | 14:12 −25:27 | 19.9 | 39.3 | 680 | [1] |
2004 NT33 | TNO | 21:23 +17:32 | 21:01 +16:00 | 20.5 | 38.5 | 457 | [2] |
(175113) 2004 PF115 | TNO | 22:46 −21:17 | 22:27 −22:51 | 20.8 | 41.5 | 468 | [1] |
(120347) Salacia | TNO | 23:15 +20:40 | 22:58 +18:47 | 20.9 | 44.3 | 901 | [1] |
(120348) 2004 TY364 | TNO | 02:49 −09:18 | 02:29 −10:24 | 20.4 | 39.3 | 489 | [2] |
(144897) 2004 UX10 | TNO | 02:36 +05:54 | 02:16 +04:17 | 20.6 | 39.0 | 398 | [1] |
2005 CC79 (2011 FX62) | TNO | 13:17 −27:28 | 12:14 −21:58 | 20.9 | 22.0 | 120 | [2] |
(303775) 2005 QU182 | TNO | 01:16 −05:38 | 01:02 −07:22 | 20.7 | 49.8 | 416 | [1] |
(145451) 2005 RM43 | TNO | 04:31 +12:06 | 04:08 +09:33 | 20.1 | 35.7 | 457 | [2] |
(145452) 2005 RN43 | TNO | 22:31 +00:57 | 22:12 −00:16 | 20.2 | 40.7 | 679 | [1] |
(145453) 2005 RR43 | TNO | 04:15 +08:43 | 03:56 +06:45 | 20.1 | 39.0 | 549 | [2] |
(202421) 2005 UQ513 | TNO | 00:37 +30:48 | 00:21 +29:09 | 20.4 | 48.5 | 724 | [2] |
2007 JH43 | TNO | 16:13 −21:05 | 15:52 −19:03 | 20.8 | 40.6 | 389 | [2] |
(278361) 2007 JJ43 | TNO | 16:24 −26:39 | 16:00 −26:33 | 20.1 | 41.4 | 575 | [2] |
(225088) 2007 OR10 | TNO | 22:23 −13:06 | 22:18 −13:50 | 21.5 | 86.7 | 1280 | [1] |
(229762) 2007 UK126 | TNO | 04:32 +00:00 | 04:14 −01:07 | 20.0 | 44.2 | 599 | [1] |
2008 OG19 | TNO | 20:33 −10:28 | 20:10 −11:11 | 20.7 | 38.6 | 417 | [2] |
2010 EK139 | TNO | 13:40 −34:54 | 13:12 −31:19 | 19.7 | 38.1 | 470 | [1] |
Notes. The classification TNO/Centaur is that adopted by the JPL. The easternmost and westernmost coordinates are an approximation of the limits within which the observations are found that covered the sky path of a given TNO, as seen from an earth-based observer, from 2012.5 to the end of 2014. The values given in the V column are just an indication of the apparent magnitudes for each object. The distances (D) are in astronomical units and refer to the JD given by Table 5. The references for the diameters are: [1] most recent value, by the time this paper was written, found in Johsnton’s archive (http://www.johnstonsarchive.net/astro/tnodiam.html); [2] determined from the values of H and G as obtained from the physical parameter area contained in the ephemerides provided by the JPL, Horizons System.
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