G5IV Garrison94 lists mu Her as the G5IV anchor standard. MK43 standard: 70 Vir - G5IV-V mu Her (=HD 161797) - G5IV JM53 standard: mu Her (=HD 161797) - G5IV MK73 dagger standard: mu Her (=HD 161797) - G5IV Keenan89 standard: mu Her (=HD 161797) - G5IV ome Sgr (=HD 188376) - G5IV Houk88 standard: mu Her (=HR 6623 = HD 161797) - G5IV [from MK73] Garrison94 anchor: mu Her (=HR 6623 = HD 161797) - G5IV GrayNstars standard: ome Sgr (=HD 188376) - G5IV mu Her - G5IV Among Gray03 and Gray06 stars within 40 pc (only HIP 42430 & 98066): B-V(G5IV) = 0.734 (+- 0.014 sem, +- 0.020 stdev; N=2) V-I(G5IV) = 0.760 (+- 0.030 sem, +- 0.042 stdev; N=2) (B-V)(G5IV) = 0.750 ; pri. stan. HD 161797 = mu Her (B-V)(G5IV) = 0.757 ; sec. stan. HD 188376 = ome Sgr (B-V)(G5IV) = 0.774 ; poly fit to FGK subgiant standards & exemplars => adopt (B-V)(G5IV) = 0.76 [updated 1/28/2022] G5IV stars w/i 60pc in SIMBAD (using SIMBAD plx, spt): Mv(G5IV) = 2.853 ; sec. stan. * ome Sgr (plx = 42.72 mas,V= 4.70) Mv(G5IV) = 2.993 ; HD 164507 (plx = 22.01 mas,V= 6.28) Mv(G5IV) = 3.09 ; quadratic trend G0IV-K2IV standards+exemplars (for G5IV) Mv(G5IV) = 3.2 ; GrayCorbally09 Mv(G5IV) = 3.775 ; HD 26729 (plx = 18.50 mas,V= 7.44) Mv(G5IV) = 3.821 ; pri. stan. * mu. Her (plx = 120.33 mas,V= 3.42) Mv(G5IV) = 3.955 ; HD 225155 (plx = 18.33 mas,V= 7.64) => adopt Mv(G5IV) = 3.09 mag [adopted 1/28/2022] Note that Sandage16 limits subgiants to a box in absolute mag space for G0-K2 and 1.6 < Mv < 3.4, but mu Her (Mv=3.82) has been considered subgiant since 1930s and Garrison94 considers it an anchor standard. Teff(G5IV) = 5530 K ; pri. stan. mu Her Teff(G5IV) = 5524 K ; sec. stan. ome Sgr => adopt Teff(G5IV) = 5530 K [updated 11/20/2019] # Primary Standards HD 161797 = mu Her = HR 6623 = HIP 86974 (J1636+4244, V=3.4) G4IV/V: Adams35 *G5IV: Keenan41,MK43,Roman52(lines weak),Keenan53(G5V+),Keenan89,Garrison94(anchor),Gray01,GrayNstars,Cannon(G5),Jaschek64(most) G5.5V: Morgan38 G8III: 1897AnHar..28....1M One of only four subgiant (IV) anchor standards (Garrison94): eta Boo (G0IV), mu Her (G5IV), bet Aql (G8IV), gam Cep (K1IV). Sandage16 mentions mu Her as one of the "six extreme subgiants with large trigonometric parallaxes... could be said to define a subgiant sequence". Has a 35" companion which itself is binary (BC: M4V,V=9.8). V=3.42(HIP), B-V=0.750+-0.015(HIP), V-Ic=0.71+-0.02(HIP). plx=119.9248+-0.1543mas(GaiaEDR3) => Mv=3.82. PASTEL values: = 5529K(N=22), <[Fe/H]>=0.24(N=20), =3.975(N=22). # Secondary Standard HD 188376 = ome Sgr = HR 7597 = HIP 98066 (J1955-2617,V=4.7) G3/5III: Houk82(#1) G4IV: 1937AnHar.105...45H *G5IV: Keenan89,Gray06 G5: Cannon G5V: Adams35 G6/8III+G: Houk82(#2) G8: Bidelman85 K0V: 1966ArA.....3..501L Houk82 notes; "HR 7597; *OMEGA SGR; OR POSSIBLY COMPOSITE G6/8 III + EARLY G". V=4.70(HIP), B-V=0.748+-0.015(HIP), B-V=0.757+-0.004(Mermilliod91), V-I=0.79(HIP). plx=42.7159+-0.5538mas(GaiaDR2) => Mv=2.85. PASTEL compendium: = 5524K(N=6), =3.82(N=4), <[Fe/H]>=0.025(N=4). # Other stars HD 143120 G5IV: Evans59,Houk78 G7IV: Lu83 HD 157347 G3V: Gray03 G5V: Harlan74 G5IV: Evans64,Cowley79