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TOI-1260

Coordinates:Sky map12h 26m 17.8916s, −51° 21′ 46.2141″
From Wikipedia, the free encyclopedia
K-type main-sequence star in the constellation Ursa Major
TOI-1260
Observation data
Epoch RA2000      Equinox RA2000
ConstellationUrsa Major
Right ascension10h 28m 35.025s[1]
Declination+65° 51′ 16.38″[1]
Apparent magnitude (V)11.875[2]
Characteristics
Evolutionary stageMain sequence
Spectral typeK6 V[2]
Astrometry
Radial velocity (Rv)−16.70±0.40[1] km/s
Proper motion (μ)RA: −177.340mas/yr[1]
Dec.: −81.693mas/yr[1]
Parallax (π)13.6226±0.0147 mas[1]
Distance239.4 ± 0.3 ly
(73.41 ± 0.08 pc)
Details[3]
Mass0.679+0.095
−0.057
 M
Radius0.672±0.010 R
Luminosity0.129±0.004 L
Surface gravity (log g)4.57±0.05 cgs
Temperature4227±85 K
Metallicity[Fe/H]−0.10±0.07 dex
Rotation30.63±3.81 d
Rotational velocity (v sin i)1.5±0.7 km/s
Age6.7+5.1
−5.2
 Gyr
Other designations
LP 62-217,NLTT 24401,TOI-1260,TIC 355867695,2MASS J10283500+6551163[4]
Database references
SIMBADdata
Exoplanet Archivedata

TOI-1260 is a single high-proper-motionK-typemain-sequencestar in theconstellation ofUrsa Major. Its surface temperature is 4227±85K. TOI-1260 has an orange hue and is too faint to be seen with thenaked eye, or a smalltelescope.[5] It has anapparent visual magnitude of 11.922±0.034. Based uponparallax measurements, it is located 239light-years from theSun. The object is drifting towards the Sun with aradial velocity of -16.7 km/s.[1]

Planetary system

[edit]

TOI-1260 has three known planets, two discovered in 2021[2] and one in 2022 by thetransit method.[6]

None of these three planets orbit in thehabitable zone. All aresub-Neptunes, with masses and radii indicating that they are partly composed of gas.[3]

The TOI-1260 planetary system[3]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b8.56±1.54 M🜨0.0367±0.00113.127463±0.000005089.03±0.61°2.41±0.05 R🜨
c13.20±4.23 M🜨0.0657±0.00207.493134±0.000020087.97±0.11°2.76±0.07 R🜨
d11.84±7.79 M🜨0.1116±0.003316.608164±0.000083089.14±0.10°3.12±0.08 R🜨

See also

[edit]

References

[edit]
  1. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcGeorgieva, I. Y.; Persson, C. M.; et al. (August 2021)."Hot planets around cool stars - two short-period mini-Neptunes transiting the late K-dwarf TOI-1260".Monthly Notices of the Royal Astronomical Society.505 (4):4684–4701.arXiv:2104.05653.Bibcode:2021MNRAS.505.4684G.doi:10.1093/mnras/stab1464.
  3. ^abcLam, K W F; Cabrera, J; Hooton, M J; Alibert, Y; Bonfanti, A; Beck, M; Deline, A; Florén, H-G; Simon, A E; Fossati, L; Persson, C M; Fridlund, M; Salmon, S; Hoyer, S; Osborn, H P (2023-02-11)."Discovery of TOI-1260d and the characterization of the multiplanet system".Monthly Notices of the Royal Astronomical Society.519 (1):1437–1451.arXiv:2212.04307.Bibcode:2023MNRAS.519.1437L.doi:10.1093/mnras/stac3639.ISSN 0035-8711.
  4. ^"LP 62-217".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2025-04-22.
  5. ^"★ TOI 1260".Stellar Catalog. Retrieved2025-04-21.
  6. ^"TOI-1260 d - NASA Science". 2022-12-23. Retrieved2025-04-21.


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