Messier 34: Perbedaan antara revisi

}}</ref> ThisIni isadalah roughlymasa-masa thedimana agebintang atdengan which stars withmassa 0.5 [[solarmassa massmatahari]]es enter thememasuki [[mainderet sequenceutama]]. ByDengan comparison,membandingkan starsbintang likeseperti the[[matahari]] Sunmemasuki enter[[deret the main sequenceutama]] aftersetelah 30 millionjuta yearstahun.<ref name="mnras370">