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  2. Red giant - Wikipedia

    en.wikipedia.org/wiki/Red_giant

    The red-giant branch variable star Gamma Crucis is the nearest M-class giant star at 88 light-years. [25] The K1.5 red-giant branch star Arcturus is 36 light-years away. [ 26 ]

  3. Lake Stars: What Are They And How Do They Form? - AOL

    www.aol.com/lake-stars-form-132029798.html

    For lake stars to form, it is believed that a thin layer of ice needs to be present with heavy snowfall on top. They begin with a single hole, and then spidery branches extend from there, creating ...

  4. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    This is the nearest red giant to the Earth, and the fourth brightest star in the night sky. Pollux (β Geminorum) 9.06 ± 0.03 [95] AD The nearest giant star to the Earth. Spica (α Virginis A) 7.47 ± 0.54 [101] One of the nearest supernova candidates and the sixteenth-brightest star in the night sky. Regulus (α Leonis A) 4.16 × 3.14 [102]

  5. The red giant star Betelgeuse is closer than we thought ... - AOL

    www.aol.com/red-giant-star-betelgeuse-closer...

    This red giant star will, one day, explode as a supernova. ... We found the second smaller event was likely due to the pulsations of the star,” Dr. Meridith ... This new study finds its body ...

  6. R Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/R_Cassiopeiae

    R Cassiopeiae is a variable star in the northern constellation of Cassiopeia. It is located approximately 570 light years distant from the Sun, but is drifting closer with a radial velocity of −23 km/s. [5] This is a pulsating Mira-type variable star with a brightness that varies from magnitude +4.4 down to +13.5 over a period of 433.6 days. [3]

  7. Detailed image of red giant confirms theory about massive stars

    www.aol.com/news/2018-01-30-detailed-image-of...

    Now, using the most detailed images of a distant star ever captured, scientists have confirmed existing theories about giant stars in the late stages of their life. The results were published in ...

  8. Red clump - Wikipedia

    en.wikipedia.org/wiki/Red_clump

    The red clump should not be confused with the "red bump" or red-giant-branch bump, which is a less noticeable clustering of giants partway along the red-giant branch, caused as stars ascending the red-giant branch temporarily decrease in luminosity because of internal convection. [10]

  9. La Superba - Wikipedia

    en.wikipedia.org/wiki/La_Superba

    La Superba is a semiregular variable star, varying by about a magnitude over a roughly 160-day cycle, but with slower variation over a larger range. Periods of 194 and 186 days have been suggested, with a resonance between the periods. [12] Y CVn is one of the reddest stars known, and it is among the brightest of the giant red carbon stars.

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