HD 70573

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Template:Short description

HD 70573
File:V478HyaLightCurve.png
A light curve for V478 Hydrae, plotted from TESS data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Hydra
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 8.66-8.77[3]
Characteristics
Evolutionary stage main sequence
Spectral type G1/2V[4]
B−V Template:Engvar 0.59[5]
Variable type BY Dra[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[2]
Dec.: Script error: No such module "val". mas/yr[2]
Parallax (π)16.9267±0.0168 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+0.4[6]
Details
MassScript error: No such module "val".[6] Template:Solar mass
RadiusScript error: No such module "val".[7] Template:Solar radius
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[6] cgs
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]Script error: No such module "val".[6] dex
Rotation3.296 days[6]
Rotational velocity (v sin i)Script error: No such module "val".[6] km/s
AgeScript error: No such module "val".[8] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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HD 70573 is a variable star in the equatorial constellation of Hydra. At a mean apparent visual magnitude of +8.7, this yellow-hued star is too dim to be visible to the naked eye. Based upon parallax measurements, it is located at a distance of 193 light years from the Sun, and is drifting further away with a radial velocity of 20.5 km/s. It is a candidate member of the proposed Hercules-Lyra Association of co-moving stars,[5] although this membership is disputed.[10]

This is a G-type main-sequence star with a stellar classification of G1/2V.[4] It is a BY Draconis variable that ranges in brightness from magnitude 8.66 down to 8.77 with a rotationally-modulated period of 3.296 days.[3] HD 70573 is generally considered to be a young star although estimates of its age vary from 60[11] million years to several billion years.[8] It has a projected rotational velocity of 15 km/s[6] and about the same mass, size, and luminosity as the Sun.

Planetary system

On March 19, 2007, an extrasolar planet was announced, having been discovered by the radial velocity method. As of 2007, this was the youngest host star discovered to have an orbiting planet.[6] However, a follow-up study by Soto et al. in 2015 failed to detect the planetary signal, so it remains unconfirmed.[12]

The system displays an infrared excess, which matches the black body signature of a debris disk orbiting Script error: No such module "val". from the host star with a mean temperature of 60 K.[13]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet hypothetical

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References

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  7. a b c Template:Cite Gaia DR2
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External links

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Template:Sky

Template:Stars of Hydra