Mira variable
Mira variables /ˈmaɪrə/ (named for the prototype star Mira) are a class of pulsating stars characterized by very red colours, pulsation periods longer than 100 days, and amplitudes greater than one magnitude in infrared and 2.5 magnitude at visual wavelengths. They are red giants in the very late stages of stellar evolution, on the asymptotic giant branch (AGB), that will expel their outer envelopes as planetary nebulae and become white dwarfs within a few million years.
Wikipage disambiguates
Wikipage redirect
Alpha LyncisAndromeda (constellation)AntliaAquila (constellation)Aries (constellation)Astronomical objectAsymptotic giant branchAuriga (constellation)BD CamelopardalisBH CrucisCW LeonisCamelopardalisCanes VenaticiCanis MinorCarina (constellation)CentaurusCentaurus ACepheus (constellation)CetusChi CygniCircumstellar envelopeComa BerenicesCorona BorealisCorvus (constellation)CruxCygnus (constellation)DelphinusDraco (constellation)EquuleusEta GeminorumFrida PalmerGottfried KirchHD 88366HV 2112Horologium (constellation)Hot bottom burningHydra (constellation)II LupiIK Tauri
Link from a Wikipage to another Wikipage
BH CrucisCW LeonisChi CygniHD 88366HV 2112II LupiIK TauriIRAS 04509-6922LL PegasiLP AndromedaeMiraR AndromedaeR AquariiR AquilaeR AurigaeR BoötisR CancriR Canum VenaticorumR CapricorniR CarinaeR CassiopeiaeR CentauriR CorviR CygniR EquuleiR FornacisR GeminorumR HorologiiR HydraeR Leonis MinorisR LeporisR NormaeR OctantisR ReticuliR SerpentisR VirginisS BoötisS Canis MinorisS CassiopeiaeS Coronae Borealis
variable
primaryTopic
Mira variable
Mira variables /ˈmaɪrə/ (named for the prototype star Mira) are a class of pulsating stars characterized by very red colours, pulsation periods longer than 100 days, and amplitudes greater than one magnitude in infrared and 2.5 magnitude at visual wavelengths. They are red giants in the very late stages of stellar evolution, on the asymptotic giant branch (AGB), that will expel their outer envelopes as planetary nebulae and become white dwarfs within a few million years.
has abstract
Die Mira-Sterne sind langperio ...... Walfisch (lat. cetus) benannt.
@de
Gwiazdy zmienne typu Mira Ceti ...... riodycznymi zmianami jasności.
@pl
Le variabili Mira sono una cla ...... le più brillanti e conosciute.
@it
Les (étoiles) variables de typ ...... carts à la symétrie sphérique.
@fr
Les variables Mira anomenades ...... des d'aproximadament un segle.
@ca
Mira izar aldakorrak gorri biz ...... atzuk ez dute esfera formarik.
@eu
Mira variables /ˈmaɪrə/ (named ...... hing back well over a century.
@en
Mira-veranderlijken of Mira-va ...... perk veel langer dan een eeuw.
@nl
Miravariabler, efter stjärnan ...... s under mer än ett århundrade.
@sv
Miridy jsou proměnné hvězdy s ...... vojhvězda v souhvězdí Velryby.
@cs
Link from a Wikipage to an external page
Wikipage page ID
page length (characters) of wiki page
Wikipage revision ID
1,025,502,558
Link from a Wikipage to another Wikipage
wikiPageUsesTemplate
subject
hypernym
comment
Die Mira-Sterne sind langperio ...... Walfisch (lat. cetus) benannt.
@de
Gwiazdy zmienne typu Mira Ceti ...... zaś staną się białymi karłami.
@pl
Le variabili Mira sono una cla ...... , e diventeranno nane bianche.
@it
Les (étoiles) variables de typ ...... rence à l'étoile Mira (o Cet).
@fr
Les variables Mira anomenades ...... es en uns pocs milions d'anys.
@ca
Mira izar aldakorrak gorri biz ...... bezala geratuko den bitartean.
@eu
Mira variables /ˈmaɪrə/ (named ...... fs within a few million years.
@en
Mira-veranderlijken of Mira-va ...... en dan een witte dwerg worden.
@nl
Miravariabler, efter stjärnan ...... dvärg inom några miljoner år.
@sv
Miridy jsou proměnné hvězdy s ...... vojhvězda v souhvězdí Velryby.
@cs
label
Estrella variable Mira
@es
Gwiazdy zmienne typu Mira Ceti
@pl
Mira izar aldakor
@eu
Mira variable
@en
Mira-Stern
@de
Mira-veranderlijke
@nl
Miravariabel
@sv
Miridy
@cs
Variabile Mira
@it
Variable Mira
@ca