2015A&A...581A.128L


Query : 2015A&A...581A.128L

2015A&A...581A.128L - Astronomy and Astrophysics, volume 581A128-128 (2015/9-1)

Detectability of quasi-circular co-orbital planets. Application to the radial velocity technique.

LELEU A., ROBUTEL P. and CORREIA A.C.M.

Abstract (from CDS):

Several celestial bodies in co-orbital configurations exist in the solar system. However, co-orbital exoplanets have not yet been discovered. This lack may result from a degeneracy between the signal induced by co-orbital planets and other orbital configurations. Here we determine a criterion for the detectability of quasi-circular co-orbital planets and develop a demodulation method to bring out their signature from the observational data. We show that the precision required to identify a pair of co-orbital planets depends only on the libration amplitude and on the planet's mass ratio. We apply our method to synthetic radial velocity data, and show that for tadpole orbits we are able to determine the inclination of the system to the line of sight. Our method is also valid for planets detected through the transit and astrometry techniques.

Abstract Copyright: ∼

Journal keyword(s): planets and satellites: detection - planets and satellites: dynamical evolution and stability - celestial mechanics

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 10180 * 01 37 53.5772394024 -60 30 41.482108548   7.95 7.32     G1V 218 2

Query : 2015A&A...581A.128L

Basic data :
HD 10180 -- Star
Other object types:
otypes_help
* (2015A&A,HD,...), NIR (2MASS)
ICRS coord. (ep=J2000) :
01 37 53.5772394024 -60 30 41.482108548 (Optical) [ 0.0133 0.0130 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
01 36 08.7129885373 -60 45 55.979027786 [ 0.0133 0.0130 90 ]
Gal coord. (ep=J2000) :
292.8053603042414 -55.6940128917121 [ 0.0133 0.0130 90 ]
Proper motions mas/yr :
-14.303 8.058 [0.017 0.016 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 35.461 [0.0004] / z(spectroscopic) 0.000118 [0.000000] / cz 35.46 [0.00]
   (Opt) A 2018A&A...616A...7S
Parallaxes (mas):
25.6611 [0.0146] A 2020yCat.1350....0G
Spectral type:
G1V C 2006AJ....132..161G
Fluxes (6) :
B 7.95 [0.01] D 2000A&A...355L..27H
V 7.32 [0.01] D 2000A&A...355L..27H
G 7.187870 [0.002761] C 2020yCat.1350....0G
J 6.246 [0.021] C 2003yCat.2246....0C
H 5.934 [0.031] C 2003yCat.2246....0C
K 5.868 [0.018] C 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 9
Display criteria :

Identifiers (22) :
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HD 10180 GSC 08850-01715 SAO 248411 uvby98 100010180
CD-61 285 HIC 7599 SKY# 2452 Gaia DR3 4716158250340258944
CPC 20.1 322 HIP 7599 SPOCS 88 Gaia DR2 4716158250340258944
CPD-61 124 2MASS J01375356-6030414 SRS 3926 Gaia DR1 4716158246044303744
GC 1984 PPM 352502 TIC 231836962
GEN# +1.00010180 RAVE J013753.6-603042 TYC 8850-1715-1

References (218 between 1850 and 2026) (Total 218)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 7    Diameter : 1    Distance : 3    Rot : 4    Fe/H : 31    Plx : 6    PM : 5    SpT : 3   

   


External archives :

Link by name to the catalogue in VizieR :

HD 10180 CD-61 285 CPD-61 124 GSC 08850-01715 HIC 7599
HIP 7599 2MASS J01375356-6030414 PPM 352502 RAVE J013753.6-603042 SAO 248411
TYC 8850-1715-1 uvby98 100010180 Gaia DR3 4716158250340258944 Gaia DR2 4716158250340258944 Gaia DR1 4716158246044303744

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