| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cetus |
| Right ascension | 23h 59m 53.8316s[1] |
| Declination | −22° 25′ 41.2159″[1] |
| Apparent magnitude (V) | 8.23[2] |
| Characteristics | |
| Spectral type | G2V[3] or G2IV[4] |
| B−V color index | 0.639±0.015[2] |
| Variable type | constant[4] |
| Astrometry | |
| Radial velocity (Rv) | 1.49±0.14[1] km/s |
| Proper motion (μ) | RA: 147.125±0.100[1] mas/yr Dec.: 26.853±0.058[1] mas/yr |
| Parallax (π) | 10.6666 ± 0.0577 mas[1] |
| Distance | 306 ± 2 ly (93.8 ± 0.5 pc) |
| Absolute magnitude (MV) | 3.29[2] |
| Details | |
| Mass | 1.29±0.09[5] M☉ |
| Radius | 1.82+0.05 −0.04[1] R☉ |
| Luminosity | 3.78±0.03[1] L☉ |
| Surface gravity (log g) | 4.18±0.06[5] cgs |
| Temperature | 5,971+55 −88[1] K |
| Metallicity [Fe/H] | 0.28±0.02[5] dex |
| Rotational velocity (v sin i) | 4.2[6] km/s |
| Age | 3.0[6] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
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.[2] 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.[1]
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.[7][8]
This is an ordinary G-type main-sequence star with a stellar classification of G2V.[3] However, in 2006, Johnson and associates assigned it a class of G2 IV, suggesting it is instead an evolving subgiant star.[4] It is about three[6] billion years old and chromospherically quiet,[4] with a projected rotational velocity of 4.2 km/s.[6] The star is metal rich, showing a higher abundance of elements other than hydrogen and helium when compared to the Sun.[4] It has 1.3[5] 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.[1]
Gaia DR2 was invoked but never defined (see the help page).Anderson2012 was invoked but never defined (see the help page).houk1978 was invoked but never defined (see the help page).Johnson2006 was invoked but never defined (see the help page).Santos2013 was invoked but never defined (see the help page).Delgado_Mena2015 was invoked but never defined (see the help page).