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HD 48948

From Wikipedia, the free encyclopedia
Star in the constellation Lynx
HD 48948
Observation data
EpochJ2000      EquinoxJ2000
ConstellationLynx
Right ascension06h 49m 57.57s[1]
Declination+60° 20′ 14.53″[1]
Apparent magnitude (V)8.58[2]
Characteristics
Evolutionary stageMain sequence star
Spectral typeK3V[3]
Apparent magnitude (J)6.33±0.02[2]
Apparent magnitude (H)5.73±0.02[2]
Apparent magnitude (K)5.61±0.02[2]
B−Vcolor index1.21[2]
Astrometry
Radial velocity (Rv)−52.061±0.0020[3] km/s
Proper motion (μ)RA: 253.401±0.020mas/yr[3]
Dec.: 410.798±0.017mas/yr[3]
Parallax (π)59.393±0.025 mas[2]
Distance54.91 ± 0.02 ly
(16.837 ± 0.007 pc)
Absolute magnitude (MV)7.46±0.05[4]
Details[2]
Mass0.686+0.020
−0.013
 M
Radius0.679±0.004 R
Luminosity0.156[5] L
Temperature4593±60 K
Metallicity[Fe/H]−0.21±0.03 dex
Rotation43.45+1
−0.71
 d
Rotational velocity (v sin i)<2 km/s
Age11.48+1.93
−4.67
 Gyr
Other designations
BD+60° 1003,Gaia DR3 1003351437484254464,HIP 32769,TYC 4097-1471-1,2MASS J06495699+6020077
Database references
SIMBADdata

HD 48948 is aK-type main-sequence star located in the constellationLynx, approximately 55light years away, based on a parallax of 59.393mas. At anapparent magnitude of 8.58, it is too faint to be seen with the naked eye.[2]

It has astellar classification of K3V, which classifies it as amain sequence star (like our Sun) fusing atoms of hydrogen into helium at its core. Estimated to be 11.5 billion years old, HD 48948 has 0.68 times themass andradius of the Sun. Its surface has aneffective temperature of 4,593 K,[2] giving it the orange glow of aK-type star.[6]

Planetary system

[edit]

In 2024, three planets were discovered orbiting HD 48948 viaradial velocity using theHARPS-N spectrograph, with orbital periods of 7.3, 38 and 151 days, respectively,[7] derived from 189 measurements over a 9.5-year period from 6 October 2013 to 16 April 2023. Of the three planets, the outermost planet, HD 48948 d, asuper-Earth weighing10.59±1.00 Earth masses, is located within thehabitable zone.[8]

The HD 48948 planetary system[2]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b>4.88±0.21 M🜨0.0652±0.00057.34013±0.000400.078+0.058
−0.050
c>7.27±0.70 M🜨0.1951±0.001637.920+0.026
−0.024
0.22+0.10
−0.11
d>10.59±1.00 M🜨0.4894±0.0042150.95+0.45
−0.41
0.12+0.12
−0.08

References

[edit]
  1. ^abVallenari, 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. ^abcdefghijDalal, S.; et al. (37) (24 June 2024)."Trio of super-Earth candidates orbiting K-dwarf HD 48948: a new habitable zone candidate".Monthly Notices of the Royal Astronomical Society.531 (4):4464–4481.doi:10.1093/mnras/stae1367.hdl:10023/30204. Retrieved9 July 2024.
  3. ^abc"HD 48948".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved9 July 2024.
  4. ^Holmberg, J.; Nordström, B.; Andersen, J. (2009-07-01). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics".Astronomy and Astrophysics.501 (3):941–947.arXiv:0811.3982.Bibcode:2009A&A...501..941H.doi:10.1051/0004-6361/200811191.ISSN 0004-6361.HD 48948's database entry atVizieR.
  5. ^McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017-10-01), "Fundamental parameters and infrared excesses of Tycho-Gaia stars",Monthly Notices of the Royal Astronomical Society,471:770–791,arXiv:1706.02208,doi:10.1093/mnras/stx1433,ISSN 0035-8711HD 48948' database entry atVizieR.
  6. ^"The Colour of Stars",Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived fromthe original on 2013-12-03, retrieved2012-01-16
  7. ^Cowing, Keith (26 June 2024)."Three Potential Super-Earths Discovered Around Nearby Star HD 48 948".Astrobiology. Retrieved11 July 2024.
  8. ^Luntz, Stephen (25 June 2024)."Nearest Super-Earth In A Habitable Zone Orbit Announced".IFLScience. Retrieved11 July 2024.
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