Q66492445
Press Enter · cited answer in seconds
0 sources
Q66492445
Summary
Q66492445 is an infrared source[1].
Key Facts
- Q66492445's instance of is recorded as infrared source[2].
- Q66492445's instance of is recorded as high proper-motion star[3].
- Q66492445's spectral class is recorded as A8IV[4].
- Q66492445's catalog code is recorded as HD 106086[5].
- Q66492445's catalog code is recorded as CPC 20 3734[6].
- Q66492445's catalog code is recorded as GSC 08974-01872[7].
- Q66492445's catalog code is recorded as HIC 59528[8].
- Q66492445's catalog code is recorded as HIP 59528[9].
- Q66492445's catalog code is recorded as 2MASS J12122535-6004041[10].
- Q66492445's catalog code is recorded as PPM 359252[11].
- Q66492445's catalog code is recorded as SAO 239751[12].
- Q66492445's catalog code is recorded as uvby98 100106086[13].
- Q66492445's catalog code is recorded as TYC 8974-1872-1[14].
- Q66492445's catalog code is recorded as Gaia DR2 6058901813222076032[15].
- Q66492445's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.06'}[16].
- Q66492445's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.82'}[17].
- Q66492445's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.7570'}[18].
- Q66492445's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.296'}[19].
- Q66492445's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.227'}[20].
- Q66492445's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.154'}[21].
- Q66492445's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.7131'}[22].
- Q66492445's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.90'}[23].
- Q66492445's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+148.9625'}[24].
- Q66492445's SIMBAD ID is recorded as HD 106086[25].
- Q66492445's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+93'}[26].