Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Eridanus |
Right ascension | 02h 52m 32.12819s [2] |
Declination | –12° 46′ 10.9681″ [2] |
Apparent magnitude (V) | 6.04 [3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | K1V [4] |
U−B color index | +1.41 [5] |
B−V color index | +0.86 [5] |
Variable type | RS CVn [6] |
Astrometry | |
Radial velocity (Rv) | +17.77±0.08 [7] km/s |
Proper motion (μ) |
RA: 397.353
[2]
mas/
yr Dec.: −189.281 [2] mas/ yr |
Parallax (π) | 96.5200 ± 0.0258 mas [2] |
Distance | 33.792 ± 0.009
ly (10.361 ± 0.003 pc) |
Absolute magnitude (MV) | 5.97 [8] |
Details | |
Mass | 0.88 [9] M☉ |
Radius | 0.85±0.05 [10] R☉ |
Luminosity | 0.408±0.005 [2] L☉ |
Surface gravity (log g) | 4.58 [9] cgs |
Temperature | 5,225±5 [11] K |
Metallicity [Fe/H] | +0.10 [12] dex |
Rotation | 6.6 days [12] |
Rotational velocity (v sin i) | 4.80 [13] km/s |
Age | 100 [14] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 17925 is a variable star in the equatorial constellation of Eridanus. It has the Gould designation 32 G. Eridani and the variable star designation EP Eri. The star has a yellow-orange hue and is dimly visible to the naked eye in good seeing conditions with an apparent visual magnitude that varies from 6.03 down to 6.08. [16] It is located nearby at a distance of 34 light years from the Sun based on parallax, [2] and is drifting further away with a radial velocity of +18 km/s. [7] It is a likely member of the Local Association of nearby, co-moving stars. [12] The spectrum shows a strong abundance of lithium, indicating that it is young star. [17] This likely makes its point of origin the nearby Scorpio–Centaurus Complex. [18]
The stellar classification of HD 17925 is K1V, [4] which indicates this is a K-type main-sequence star that is engaged in core hydrogen fusion. It is an active star [17] that is classified as a RS Canum Venaticorum variable, [16] showing a rotational modulation with a period of 6.9 days, and has been observed to flare. [6] The star has an estimated age of 100 [14] million years and is spinning with a projected rotational velocity of 4.8 km/s. [13] The rotation period of 6.6 days days can be determined from its activity cycle. [12] The star has 88% [9] of the mass of the Sun and 85% [10] of the Sun's radius. It is radiating 41% [2] of the luminosity of the Sun from its photosphere at an effective temperature of 5,225 K. [11]
The presence of an unseen companion has been suggested based on variations in the widths of absorption lines in the star's photosphere. [17] It displays low-amplitude radial velocity variation, which may indicate it is a spectroscopic binary. [10] However, the binary hypothesis doesn't appear to be consistent with Hipparcos satellite data. [12] An infrared excess has been detected around this star, most likely indicating the presence of a circumstellar disk at a radius of 17.9 AU. The temperature of this dust is 52 K. [19]
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: CS1 maint: multiple names: authors list (
link)Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Eridanus |
Right ascension | 02h 52m 32.12819s [2] |
Declination | –12° 46′ 10.9681″ [2] |
Apparent magnitude (V) | 6.04 [3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | K1V [4] |
U−B color index | +1.41 [5] |
B−V color index | +0.86 [5] |
Variable type | RS CVn [6] |
Astrometry | |
Radial velocity (Rv) | +17.77±0.08 [7] km/s |
Proper motion (μ) |
RA: 397.353
[2]
mas/
yr Dec.: −189.281 [2] mas/ yr |
Parallax (π) | 96.5200 ± 0.0258 mas [2] |
Distance | 33.792 ± 0.009
ly (10.361 ± 0.003 pc) |
Absolute magnitude (MV) | 5.97 [8] |
Details | |
Mass | 0.88 [9] M☉ |
Radius | 0.85±0.05 [10] R☉ |
Luminosity | 0.408±0.005 [2] L☉ |
Surface gravity (log g) | 4.58 [9] cgs |
Temperature | 5,225±5 [11] K |
Metallicity [Fe/H] | +0.10 [12] dex |
Rotation | 6.6 days [12] |
Rotational velocity (v sin i) | 4.80 [13] km/s |
Age | 100 [14] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 17925 is a variable star in the equatorial constellation of Eridanus. It has the Gould designation 32 G. Eridani and the variable star designation EP Eri. The star has a yellow-orange hue and is dimly visible to the naked eye in good seeing conditions with an apparent visual magnitude that varies from 6.03 down to 6.08. [16] It is located nearby at a distance of 34 light years from the Sun based on parallax, [2] and is drifting further away with a radial velocity of +18 km/s. [7] It is a likely member of the Local Association of nearby, co-moving stars. [12] The spectrum shows a strong abundance of lithium, indicating that it is young star. [17] This likely makes its point of origin the nearby Scorpio–Centaurus Complex. [18]
The stellar classification of HD 17925 is K1V, [4] which indicates this is a K-type main-sequence star that is engaged in core hydrogen fusion. It is an active star [17] that is classified as a RS Canum Venaticorum variable, [16] showing a rotational modulation with a period of 6.9 days, and has been observed to flare. [6] The star has an estimated age of 100 [14] million years and is spinning with a projected rotational velocity of 4.8 km/s. [13] The rotation period of 6.6 days days can be determined from its activity cycle. [12] The star has 88% [9] of the mass of the Sun and 85% [10] of the Sun's radius. It is radiating 41% [2] of the luminosity of the Sun from its photosphere at an effective temperature of 5,225 K. [11]
The presence of an unseen companion has been suggested based on variations in the widths of absorption lines in the star's photosphere. [17] It displays low-amplitude radial velocity variation, which may indicate it is a spectroscopic binary. [10] However, the binary hypothesis doesn't appear to be consistent with Hipparcos satellite data. [12] An infrared excess has been detected around this star, most likely indicating the presence of a circumstellar disk at a radius of 17.9 AU. The temperature of this dust is 52 K. [19]
{{
citation}}
: CS1 maint: multiple names: authors list (
link)