Examples of using Variable star in English and their translations into Portuguese
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Official/political
Variable star obs.
It is a suspected variable star.
The variable star designation for HD 209458 is V376 Pegasi.
It is an irregular variable star.
DY Centauri is a variable star in the constellation Centaurus.
It is classified as a BY Draconis type variable star.
AE Phoenicis is a variable star in the constellation of Phoenix.
The asymmetrical appearance of Mira, an oscillating variable star.
R And is a Mira-type variable star with a period of 409 days.
Retrieved 22 May 2014."* Gamma Serpentis- Variable star.
A0620-00 also bears the variable star designation V616 Monocerotis.
Like many low-mass stars, Gliese 876 is a variable star.
Chi Cygni(χ Cyg, χ Cygni)is a variable star of the Mira type in the constellation Cygnus.
Light Curve produced by the American Amateur Variable Star Observers.
A Delta Cephei type variable star designated"U Sagittarii" is a member of this cluster.
AAVSO- American Association of Variable Star Observers.
It is a Delta Scuti variable star with a period of 0.0960 days and an amplitude of 0.020 in magnitude.
U Orionis(abbreviated U Ori)is a Mira-type variable star in the constellation Orion.
Being a new variable star, it was designated V838 Monocerotis, the 838th variable star of Monoceros.
He is best known for his observations of the variable star Algol(Beta Persei) in 1782.
A flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes.
Rotating ellipsoidal variables are a class of variable star.
The result is a type of extrinsic variable star system called an eclipsing binary.
A is a Gamma Cassiopeiae type variable star and the system's brightness varies from magnitude +3.58 to +3.78.
The SuperWASP project has observed andclassified this star as a variable star, perhaps due to the eclipsing planet.
It is categorized as a Delta Scuti variable star and it has a periodic cycle of luminosity variation that repeats itself about 22.9 times per day.
Opens the AAVSO Light Curve Generator Tool, which allows you to download a light curve for any variable star from the American Association of Variable Star Observers.
Antares is a type"LC" slow irregular variable star, whose apparent magnitude slowly varies from +0.88 to +1.16.
Some of these correspond to the known Miras and semi-regulars, butan additional class of variable star has been defined: OGLE Small Amplitude Red Giants or OSARGs.
Luyten 726-8B is also known under the variable star designation UV Ceti, being the archetype for the class of flare stars. .