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HD 69830 information


HD 69830
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Puppis
Right ascension 08h 18m 23.94697s[1]
Declination −12° 37′ 55.8172″[1]
Apparent magnitude (V) +5.98[2]
Characteristics
Spectral type G8V[3]
U−B color index 0.33[2]
B−V color index 0.75[2]
V−R color index 0.40
R−I color index 0.36
Variable type none
Astrometry
Radial velocity (Rv)30.09±0.12[1] km/s
Proper motion (μ) RA: 278.790 mas/yr[1]
Dec.: −987.829 mas/yr[1]
Parallax (π)79.4953 ± 0.0400 mas[1]
Distance41.03 ± 0.02 ly
(12.579 ± 0.006 pc)
Absolute magnitude (MV)5.47 ± 0.01[4]
Details
Mass0.89 ± 0.03[5] M
Radius0.905 ± 0.019[3] R
Luminosity0.622 ± 0.014[3] L
Surface gravity (log g)4.53[6] cgs
Temperature5,394 ± 62[3] K
Metallicity [Fe/H]−0.04 ± 0.03[3] dex
Rotation35.1 ± 0.8 days[7]
Rotational velocity (v sin i)0.8±0.5[3] km/s
Age10.6 ± 4[3] Gyr
Other designations
285 G. Puppis,[8] BD−12°2449, GJ 302, HIP 40693, HR 3259, LHS 245, SAO 154093, 2MASS J08182389-1237541, Gaia DR2 5726982995343100928[9]
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata

HD 69830 (285 G. Puppis) is a yellow dwarf star located 41.0 light-years (12.6 parsecs) away in the constellation of Puppis. In 2005, the Spitzer Space Telescope discovered a narrow ring of warm debris orbiting the star.[10] The debris ring contains substantially more dust than the Solar System's asteroid belt. In 2006, three extrasolar planets with minimum masses comparable to Neptune were confirmed in orbit around the star, located interior to the debris ring.[11]

  1. ^ a b c d e Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  2. ^ a b c Cite error: The named reference MERMILLIOD was invoked but never defined (see the help page).
  3. ^ a b c d e f g Cite error: The named reference apj800_2_115 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference Holmberg2009 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Laliotis2023 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference apj764_1_78 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference mnras408_3_1666 was invoked but never defined (see the help page).
  8. ^ Benjamin Apthorp Gould, reprinted; updated by Frederick Pilcher. "Uranometria Argentina". Archived from the original on 2012-02-27. Retrieved 2011-02-04.
  9. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference Beichman2005 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Lovis2006 was invoked but never defined (see the help page).

and 24 Related for: HD 69830 information

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HD 69830

Last Update:

HD 69830 (285 G. Puppis) is a yellow dwarf star located 41.0 light-years (12.6 parsecs) away in the constellation of Puppis. In 2005, the Spitzer Space...

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HD 69830 d

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HD 69830 d is an exoplanet likely orbiting within the habitable zone of the star HD 69830, the outermost of three such planets discovered in the system...

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HD 69830 b

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HD 69830 b is a Neptune-mass or super-Earth-mass exoplanet orbiting the star HD 69830. It is at least 10 times more massive than Earth. It also orbits...

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Solar System belts

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have no asteroid belts or one vast asteroid belt. The stars Fomalhaut, HD 69830 and Epsilon Eridani are examples of systems with one large asteroid belt...

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HD 69830 c

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HD 69830 c is an exoplanet orbiting HD 69830. It is the second-closest planet in its system and has a minimum mass 12 times that of Earth. Based on theoretical...

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Debris disk

Last Update:

Wyatt, M. C. (2007). "On the Nature of the Dust in the Debris Disk around HD 69830". The Astrophysical Journal. 658 (1): 584–592. arXiv:astro-ph/0611452....

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Solar analog

Last Update:

- Bibliography - Image. HD 69830 at SIMBAD - Ids - Bibliography - Image. HD 10307 at SIMBAD - Ids - Bibliography - Image. HD 147513 at SIMBAD - Ids -...

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Habitable zone

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place. HD 69830 d, a gas giant with 17 times the mass of Earth, was found in 2006 orbiting within the circumstellar habitable zone of HD 69830, 41 light...

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Puppis

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orbiting the star HD 70642. This planetary system is much like Jupiter with a wide, circular orbit and a long-period. On May 17, 2006, HD 69830 (the nearest...

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HD 23079 b

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planet's orbital eccentricity is about the same as 109 Piscium b, HD 75898 b, and HD 69830 b at 0.102. The distance range from as close as 1.44 AU to as far...

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High Accuracy Radial Velocity Planet Searcher

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discoveries from HARPS HARPS spectrograph HARPS spectrograph detail Animation of HD 10180 with its seven planets Similar instruments: HARPS-N is a copy of this...

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List of stars in Puppis

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Hipparcos and Tycho Catalogues". Retrieved 2006-12-26. Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 2006-12-26. Roman, N...

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Embryo space colonization

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Artist's impression from 2005 of the planet HD 69830 d. Embryo space colonization depends on the existence of a habitable terrestrial exoplanet....

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List of nearest bright stars

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−44° 24′ 18.7″ 40.8 ρ1 Cancri A G8V 5.96 5.47 08h 52m 35.85s +28° 19′ 50.9″ 40.9 HD 69830 (285 G. Puppis) K0V 5.95 5.45 08h 18m 23.62s −12° 37′ 55.8″ 41.0 Gliese...

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Zeta Leporis

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years ago, peaking with an apparent magnitude of -2.05. Delta Trianguli HD 69830 Vega van Leeuwen, F. (November 2007). "Validation of the new Hipparcos...

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List of multiplanetary systems

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Jupiter mass dividing line. 54 Piscium (HD 3651) HD 168443 Gliese 229 A Epsilon Indi A HD 82943 Pi Mensae HD 38529 HD 245134 Lists of exoplanets Methods of...

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HD 169830

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the star. In 2022, the inclination and true mass of HD 169830 c were measured via astrometry. HD 69830 List of extrasolar planets Vallenari, A.; et al. (Gaia...

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Discoveries of exoplanets

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dimness of the star, the planet is probably the coldest exoplanet known. HD 69830: Has a planetary system with three Neptune-mass planets. It is the first...

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HD 109271

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2013. These are close to a 1:4 resonance, so the system is similar to HD 69830. A third Neptune in the Venus zone was hypothesised from the data. These...

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List of exoplanets detected by radial velocity

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most massive exoplanet candidate is HD 217786 b, which masses 12.98 MJ; the least massive confirmed planet is HD 10180 b, which masses 0.004 MJ or 3.1...

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HD 60532

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The orbital periods of these two planets appear to be in 3:1 resonance. HD 69830 List of extrasolar planets Vallenari, A.; et al. (Gaia collaboration) (2023)...

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HIP 57274 d

Last Update:

its own magnetosphere, even though its mass is only 0.025 ME. Kepler-90h HD 69830 d Kepler-47c "Planet HIP 57274 d". Extrasolar Planets Encyclopaedia. Retrieved...

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Omicron Puppis

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an asterism consisting of ο Puppis, δ Canis Majoris, η Canis Majoris, HD 63032, HD 65456, k Puppis, ε Canis Majoris, κ Canis Majoris and π Puppis. Consequently...

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Nu Puppis

Last Update:

Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts...

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