S Serpentis
variable star in the constellation Serpens
Press Enter · cited answer in seconds
0 sources
S Serpentis
Summary
S Serpentis is a Mira variable[1].
Key Facts
- S Serpentis's instance of is recorded as Mira variable[2].
- S Serpentis's instance of is recorded as long-period variable star[3].
- S Serpentis's instance of is recorded as astrophysical maser[4].
- S Serpentis's constellation is recorded as Serpens[5].
- S Serpentis's spectral class is recorded as M5e[6].
- S Serpentis's catalog code is recorded as ASAS J152139+1418.8[7].
- S Serpentis's catalog code is recorded as DO 15222[8].
- S Serpentis's catalog code is recorded as GCRV 8889[9].
- S Serpentis's catalog code is recorded as HD 136695[10].
- S Serpentis's catalog code is recorded as HIC 75170[11].
- S Serpentis's catalog code is recorded as HIP 75170[12].
- S Serpentis's catalog code is recorded as IRAS 15193+1429[13].
- S Serpentis's catalog code is recorded as IRC +10290[14].
- S Serpentis's catalog code is recorded as 2MASS J15213955+1418532[15].
- S Serpentis's catalog code is recorded as RAFGL 1765[16].
- S Serpentis's catalog code is recorded as SAO 101503[17].
- S Serpentis's catalog code is recorded as BD+14 2864[18].
- S Serpentis's catalog code is recorded as TYC 939-6-1[19].
- S Serpentis's catalog code is recorded as WEB 12823[20].
- S Serpentis's catalog code is recorded as Gaia DR2 1182936630152095104[21].
- S Serpentis's catalog code is recorded as S Ser[22].
- S Serpentis's type of variable star is recorded as long-period variable star[23].
- S Serpentis's type of variable star is recorded as Mira variable[24].
- S Serpentis's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.37'}[25].
- S Serpentis's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.37'}[26].
Body
Designation and Status
Recorded instance of include Mira variable[2], long-period variable star[3], and astrophysical maser[4].
History and Context
Catalog codes include ASAS J152139+1418.8[7], DO 15222[8], GCRV 8889[9], HD 136695[10], HIC 75170[11], and HIP 75170[12].