HD 195689
star in the constellation Cygnus
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HD 195689
Summary
HD 195689 is a star[1].
Key Facts
- HD 195689's image is recorded as PIA21472 - Hottest Hot Jupiter Animation (Artist's Concept), Figure 1.jpg[2].
- HD 195689's instance of is recorded as star[3].
- HD 195689's instance of is recorded as spectroscopic binary[4].
- HD 195689's instance of is recorded as eclipsing binary star[5].
- HD 195689's instance of is recorded as near-infrared source[6].
- HD 195689's instance of is recorded as ultraviolet source[7].
- HD 195689's constellation is recorded as Cygnus[8].
- HD 195689's spectral class is recorded as A0[9].
- HD 195689's part of is recorded as Q74167936[10].
- HD 195689's child astronomical body is recorded as KELT-9 b[11].
- HD 195689's catalog code is recorded as HD 195689[12].
- HD 195689's catalog code is recorded as CEL 5094[13].
- HD 195689's catalog code is recorded as GSC 03157-00638[14].
- HD 195689's catalog code is recorded as HIC 101252[15].
- HD 195689's catalog code is recorded as HIP 101252[16].
- HD 195689's catalog code is recorded as 2MASS J20312634+3956196[17].
- HD 195689's catalog code is recorded as PPM 85104[18].
- HD 195689's catalog code is recorded as SAO 70152[19].
- HD 195689's catalog code is recorded as TD1 26880[20].
- HD 195689's catalog code is recorded as UBV 17807[21].
- HD 195689's catalog code is recorded as uvby98 100195689[22].
- HD 195689's catalog code is recorded as AG+39 2158[23].
- HD 195689's catalog code is recorded as BD+39 4221[24].
- HD 195689's catalog code is recorded as Gaia DR1 2064327274354331520[25].
- HD 195689's catalog code is recorded as Gaia DR2 2064327278651198336[26].
Body
Geography
HD 195689's part of is recorded as Q74167936[10].
Designation and Status
Recorded instance of include star[3], spectroscopic binary[4], eclipsing binary star[5], near-infrared source[6], and ultraviolet source[7].
History and Context
Catalog codes include HD 195689[12], CEL 5094[13], GSC 03157-00638[14], HIC 101252[15], HIP 101252[16], and 2MASS J20312634+3956196[17].