V960 Herculis

Summary

V960 Herculis is a long-period variable star^[1].

Key Facts

• V960 Herculis's instance of is recorded as long-period variable star^[2].
• V960 Herculis's instance of is recorded as near-infrared source^[3].
• V960 Herculis's constellation is recorded as Hercules^[4].
• V960 Herculis's spectral class is recorded as K5^[5].
• V960 Herculis's catalog code is recorded as DO 16152^[6].
• V960 Herculis's catalog code is recorded as GSC 02610-00433^[7].
• V960 Herculis's catalog code is recorded as GSC 02610-00182^[8].
• V960 Herculis's catalog code is recorded as HD 160541^[9].
• V960 Herculis's catalog code is recorded as HIC 86392^[10].
• V960 Herculis's catalog code is recorded as HIP 86392^[11].
• V960 Herculis's catalog code is recorded as IRAS 17372+3154^[12].
• V960 Herculis's catalog code is recorded as 2MASS J17390949+3153106^[13].
• V960 Herculis's catalog code is recorded as PPM 80440^[14].
• V960 Herculis's catalog code is recorded as SAO 66218^[15].
• V960 Herculis's catalog code is recorded as AG+31 1540^[16].
• V960 Herculis's catalog code is recorded as BD+31 3071^[17].
• V960 Herculis's catalog code is recorded as Gaia DR1 4600886993177991552^[18].
• V960 Herculis's catalog code is recorded as Gaia DR2 4600886997474136448^[19].
• V960 Herculis's catalog code is recorded as V960 Her^[20].
• V960 Herculis's catalog code is recorded as TIC 18232709^[21].
• V960 Herculis's catalog code is recorded as Gaia DR3 4600886997474136448^[22].
• V960 Herculis's catalog code is recorded as TYC 2610-433-1^[23].
• V960 Herculis's type of variable star is recorded as SRd semi-regular variable star^[24].
• V960 Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.99'}^[25].
• V960 Herculis's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.46'}^[26].

Body

Designation and Status

Recorded instance of include long-period variable star^[2] and near-infrared source^[3].

History and Context

Catalog codes include DO 16152^[6], GSC 02610-00433^[7], GSC 02610-00182^[8], HD 160541^[9], HIC 86392^[10], and HIP 86392^[11].