HD 224693

HD 224693, also named Axólotl, is a star in the equatorial constellation of Cetus, and is positioned near the western constellation border with Aquarius. It can be viewed with a small telescope but is too faint to be seen with the naked eye, having an apparent visual magnitude of 8.23. Based on parallax measurements, the object is located at a distance of approximately 306 light years from the Sun. It is drifting further away with a radial velocity of 1.5 km/s.

HD 224693 / Axólotl
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus
Right ascension 23h 59m 53.8316s
Declination −22° 25 41.2159
Apparent magnitude (V) 8.23
Characteristics
Spectral type G2V or G2IV
B−V color index 0.639±0.015
Variable type constant
Astrometry
Radial velocity (Rv)1.49±0.14 km/s
Proper motion (μ) RA: 147.125±0.100 mas/yr
Dec.: 26.853±0.058 mas/yr
Parallax (π)10.6666 ± 0.0577 mas
Distance306 ± 2 ly
(93.8 ± 0.5 pc)
Absolute magnitude (MV)3.29
Details
Mass1.29±0.09 M
Radius1.82+0.05
−0.04
 R
Luminosity3.78±0.03 L
Surface gravity (log g)4.18±0.06 cgs
Temperature5,971+55
−88
 K
Metallicity [Fe/H]0.28±0.02 dex
Rotational velocity (v sin i)4.2 km/s
Age3.0 Gyr
Other designations
Axólotl, CD−23°18108, HD 224693, HIP 118319, SAO 192301
Database references
SIMBADdata

The star HD 224693 is named Axólotl. The name was selected in the NameExoWorlds campaign by Mexico, during the 100th anniversary of the IAU. "Axólotl" means "water animal" in the native Nahuatl language and an axolotl is also a species of salamander endemic to the valley of Mexico.

This is an ordinary G-type main-sequence star with a stellar classification of G2V. However, in 2006, Johnson and associates assigned it a class of G2 IV, suggesting it is instead an evolving subgiant star. It is about three billion years old and chromospherically quiet, with a projected rotational velocity of 4.2 km/s. The star is metal rich, showing a higher abundance of elements other than hydrogen and helium when compared to the Sun. It has 1.3 times the mass of the Sun and 1.8 times the Sun's radius. The star is radiating 3.78 times the luminosity of the Sun from its photosphere at an effective temperature of 5,971 K.

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