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- 24 mar. 05: Planet e challanged; Neptune-sized planet at ~ 0.8 AU? (Wisdom, 2005)
- 20 apr. 03: Planet in wide (a ~ 1065 AU) binary system (Eggenberger et al 2003)
- 12 Feb. 03 55 Cnc is one of the 5 targets of the 14 Feb. 03
"Cosmic Call" initiative
- 13 Jun. 02 Periodicity at 44 d. could be due to stellar rotation, but the planet interpretation is more likely (Marcy et al 2002)
- 4 Dec. 01:From astrometry with HST (McGrath et al 2002), M < 30 MJ
- 22 Nov. 00: From astrometry (Han et al. 2000) claim a preliminary mass of 126 MJ and inclination of 179.6o
- Exhibits coherent variations in residual velocities
consistent with additional companion.
24 Jul. 00: the source of RV variation remains speculative,
depending on completion of one full orbit (Fischer et al 2000).
- Possible second companion; see Butler et al. 1996, Jayawardhana et al. 2000.
- The star is surrounded by a dust disk extending at least a 40 AU, with an inclination of ~ 25o. If the planets are in the
same plane than the disc, this gives to the first planet a mass of 1.9+1.1
-0.4 MJ (Trilling & Brown 1998, Trilling et al 2000). But disc not confirmed by Schneider et al (2000b)
There may by a hole with a radius of ~ 10 AU in the disk (Jayawardhana et al 2000)
- The star has a companion (rho Cnc B) about 1150 AU away
- 24 mar. 05: Planet e challanged; Neptune-sized planet at ~ 0.8 AU? (Wisdom, 2005)
- 20 apr. 03: Planet in wide (a ~ 1065 AU) binary system (Eggenberger et al 2003)
- 13 Jun. 02 Periodicity at 44 d. could be due to stellar rotation, but the planet interpretation is more likely (Marcy et al 2002)
- 4 Dec. 01:From astrometry with HST (McGrath et al 2002), M < 30 MJ
- 22 Nov. 00: From astrometry (Han et al. 2000) claim a preliminary mass of 126 MJ and inclination of 179.6o
- Exhibits coherent variations in residual velocities
consistent with additional companion.
24 Jul. 00: the source of RV variation remains speculative,
depending on completion of one full orbit (Fischer et al 2000).
- Possible second companion; see Butler et al. 1996, Jayawardhana et al. 2000.
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