us ▁and ▁an ▁out lying ▁member ▁of ▁the ▁Hy ades ▁star ▁cluster . ▁It ▁is ▁visible ▁to ▁the ▁n aked ▁eye ▁with ▁an ▁apparent ▁visual ▁magnitude ▁of ▁ 4 . 6 2 , ▁and ▁is ▁located ▁at ▁an ▁estimated ▁distance ▁of ▁about ▁ 1 7 3   light ▁years ▁based ▁upon ▁par alla x ▁measurements . ▁The ▁star ▁is ▁moving ▁away ▁from ▁the ▁Sun ▁with ▁a ▁radial ▁velocity ▁of ▁+ 3 8   km / s . ▁ ▁This ▁has ▁been ▁reported ▁as ▁a ▁double ▁star ▁with ▁two ▁components ▁at ▁separation ▁ 0 . 1 ", ▁both ▁of ▁type ▁A 7 V ▁and ▁magnitude ▁ 5 . 4 . ▁The ▁combined ▁spectrum ▁matches ▁a ▁stell ar ▁classification ▁of ▁A 7   V , ▁which ▁would ▁normally ▁indicate ▁an ▁A - type ▁main - sequence ▁star ▁that ▁is ▁generating ▁energy ▁through ▁hydro gen ▁fusion ▁at ▁its ▁core . ▁It ▁has ▁an ▁estimated ▁age ▁of ▁ 7 1 7   mill ion ▁years . ▁ ▁References ▁ ▁Category : A - type ▁main - sequence ▁stars ▁Category : Hy ades ▁( star ▁cluster ) ▁Ta uri , ▁I ota ▁Category : T aur us ▁( const ell ation ) ▁B D + 2 1 ▁ 0 7 5 1 ▁Ta uri , ▁ 1 0 2 ▁ 0 3 2 3 0 1 ▁ 0 2 3 4 9 7 ▁ 1 6 2 0 <0x0A> </s> ▁The ▁ 2 0 0 4 ▁Pitts burgh ▁Ste el ers ▁season ▁ ▁was ▁the ▁franch ise '