TY Herculis
variable star
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TY Herculis
Summary
TY Herculis is a long-period variable star[1].
Key Facts
- TY Herculis's instance of is recorded as long-period variable star[2].
- TY Herculis's instance of is recorded as infrared source[3].
- TY Herculis's instance of is recorded as near-infrared source[4].
- TY Herculis's constellation is recorded as Hercules[5].
- TY Herculis's spectral class is recorded as M0[6].
- TY Herculis's catalog code is recorded as AG+13 1587[7].
- TY Herculis's catalog code is recorded as BD+13 3174[8].
- TY Herculis's catalog code is recorded as GSC 00973-01275[9].
- TY Herculis's catalog code is recorded as HIC 81291[10].
- TY Herculis's catalog code is recorded as HIP 81291[11].
- TY Herculis's catalog code is recorded as IRAS 16338+1324[12].
- TY Herculis's catalog code is recorded as PPM 132488[13].
- TY Herculis's catalog code is recorded as SAO 102266[14].
- TY Herculis's catalog code is recorded as YZ 13 5791[15].
- TY Herculis's catalog code is recorded as 2MASS J16361164+1318450[16].
- TY Herculis's catalog code is recorded as Gaia DR1 4461192597758966144[17].
- TY Herculis's catalog code is recorded as Gaia DR2 4461192602057335424[18].
- TY Herculis's catalog code is recorded as TY Her[19].
- TY Herculis's catalog code is recorded as TIC 148164816[20].
- TY Herculis's catalog code is recorded as Gaia DR3 4461192602057335424[21].
- TY Herculis's catalog code is recorded as TYC 973-1275-1[22].
- TY Herculis's type of variable star is recorded as long-period variable star[23].
- TY Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.88'}[24].
- TY Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.28'}[25].
- TY Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.228'}[26].
Body
Designation and Status
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].
History and Context
Catalog codes include AG+13 1587[7], BD+13 3174[8], GSC 00973-01275[9], HIC 81291[10], HIP 81291[11], and IRAS 16338+1324[12].