id: Partikel Beta

id: Beta Carinae

id: Beta Centauri

id: Beta Geminorum

; < span id =" beta "> Beta </ span >: Advice on how to successfully complete ( or protect ) a particular climbing route, boulder problem, or crux sequence.

; < span id =" beta_flash "> Beta flash </ span >: The clean ascent of a climb on the first attempt, having previously obtained beta or while having beta shouted up from the ground en route.

id: Beta Canis Minoris

id: Beta Andromedae

TeamTNT originally formed as a two-group entity: the Alpha group whose concerns centered primarily on level design and mod work employing pre-existing Doom II resources as developed by the original id software team, and the Beta group who would be focused more closely on partial and total conversions including sprite changes.

The Beta team dissolved shortly after the official formation of The TeamTNT Trust, the legal entity which dealt with id software during negotiations concerning Final Doom.

id: Beta Hydri

id: Beta Leonis

id: Mesin Beta Hyundai

id: Beta Aurigae

id: Beta Cassiopeiae

id: Beta Pegasi

id: Beta Ceti

id: Beta Librae

id: Beta Lyrae

id: Beta Eridani

id: Beta Ophiuchi

id: Beta Cancri

id: Beta Capricorni

id: Beta Draconis

id: Delta Crucis

The four main stars that form the asterism are Alpha, Beta, Gamma, and Delta Crucis.

Beta Crucis, called Mimosa, is a blue-hued giant of magnitude 1. 3, 353 light-years from Earth.

The southern celestial pole lies at the intersection of ( a ) the line along the long axis of crux ( i. e. through Alpha Crucis and Gamma Crucis ) and ( b ) a line perpendicularly bisecting the line joining the " Pointers " ( Alpha Centauri and Beta Centauri ).

Beta Crucis, also known as Mimosa or Becrux, is the second brightest star in the constellation Crux ( after Alpha Crucis or Acrux ) and is the 19th brightest star in the night sky.

Although Beta Crucis, " Becrux ", is at roughly − 60 ° declination, and therefore not visible north of 30 °, in the time of the ancient Greeks and Romans it was visible north of 40 ° due to the precession of equinoxes, and these civilizations regarded it as part of the constellation Centaurus.

Beta Crucis is believed to be the hottest first-magnitude star, with an apparent visual magnitude of 1. 25.

The primary, Beta Crucis A, is a massive star with about 16 times the Sun's mass.

Beta Crucis A is a known Beta Cephei variable, although with an effective temperature of about 27, 000 K it is at the high end of the instability strip where such stars are found.

The Beta Crucis system may be a member of the Lower Centaurus-Crux sub-group of the Scorpius-Centaurus Association.

Crucis, Beta

br: Beta Crucis

fr: Beta Crucis

la: Beta Crucis

fi: Beta Crucis

Thus Beta Crucis appears to the right of the constellation and Delta Crucis to the left, in mirror image of the way they actually appear in the sky ( and, coincidentally, the way they appear on the Brazilian coat of arms ).

The cluster looks like a star to the unaided eye and appears close to the easternmost star of the Southern Cross, ( Beta Crucis ), so is only visible from southern latitudes.

The Jewel Box cluster can be easily located using the star Beta Crucis as a guide, and appears as a fourth magnitude object.

Delta Crucis is a strong candidate Beta Cephei variable and changes its brightness subtly with a period of 1. 3 hours.

# redirect Beta Crucis