irregular variable वाक्य
उदाहरण वाक्य
मोबाइल
- Some semiregular and irregular variables are less luminous giant stars, while others are more luminous supergiants including some of the VY CMa.
- It is classified as a slow irregular variable and its brightness varies from magnitude + 4.75 to + 4.93.
- BE Camelopardalis is a red irregular variable star and its brightness varies from magnitude + 4.35 to + 4.48.
- V520 Carinae is an orange irregular variable star and its brightness varies from magnitude + 4.63 to + 4.70.
- It has never been observed since, but that does not preclude the possibility of it being a highly irregular variable star or a recurrent nova.
- It is classified as an slow irregular variable of type LC and its brightness varies from magnitude + 4.24 to + 4.34.
- Lambda Pavonis is a bright irregular variable ranging between magnitudes 3.4 and 4.4; this variation can be observed with the unaided eye.
- This star is a slow irregular variable of type LB . Its brightness varies between K, meaning it is brighter, yet cooler, than the Sun.
- Antares is a type " LC " slow irregular variable star, whose apparent magnitude slowly varies from + 0.6 to + 1.6.
- R Coronae Australis is an irregular variable star ranging from magnitudes 9.7 to 13.9 . Blue-white, it is of spectral type B5IIIpe.
- At its broadest, LPVs include Mira, semiregular, slow irregular variables, and OGLE small amplitude red giants ( OSARGs ), including both giant and supergiant stars.
- It is an irregular variable with seven measured pulsation periods ranging from 22.4 to 162.6 days, and amplitudes ranging up to 0 . m 022.
- It has been given the sub-classification of Lc " Irregular variable supergiants of late spectral types having amplitudes of about 1 mag . in V . O ".
- Another irregular variable, RX Telescopii is a red supergiant that varies between magnitudes 6.45 and 7.47, just visible to the unaided eye under good viewing conditions.
- It is an irregular variable located approximately 9, 000 light-years away from the Sun, and is currently considered one of the largest known stars, with a radius estimate of.
- It is a red giant of spectral type M3III . It has been classified as a slow irregular variable, after being found to be slightly variable in 1969 by Olin J . Eggen.
- This is a massive supergiant star with a stellar classification of M0 I . It is a slow irregular variable of the LC type, with its brightness varying in magnitude by 0.44.
- To the northwest lies Mu Muscae, an orange giant of spectral type K4III that varies between apparent magnitude is 4.71 and 4.76 and has been classified as a slow irregular variable.
- It is an irregular variable whose apparent visual magnitude varies between 4.45 and 4.64, and, at its brightest, it is the brightest of the four stars in the Terebellum.
- It is a slow irregular variable star with a possible period of 3, 100 days . It is approximately 69, 000 times the luminosity of the Sun, and it is 645 times bigger than the Sun.
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