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Mira as seen by the Hubble Space Telescope in August 1997. Mira A is a variable star, specifically the prototypical Mira variable. The 6,000 to 7,000 known stars of this class [24] are all red giants whose surfaces pulsate in such a way as to increase and decrease in brightness over periods ranging from about 80 to more than 1,000 days.
Mira, the prototype of the Mira variables. Mira variables / ˈ m aɪ r ə / (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. [1]
The Mira Loma National Science Bowl team (consisting of a group of students that answer gameshow-style questions on science and mathematics) won the national championship in 2009, 2011, 2013, 2014, and 2015. With five victories, the school has more than any other in the history of Science Bowl, and their 3-year win streak is the second-longest ...
The bonus question is always in the same category as the corresponding toss-up question, though it may not always relate to the toss-up question. Since only one team has the opportunity to answer the bonus question, there is no need to buzz in to answer it. After the moderator finishes reading the question, the team has 20 seconds to answer.
1. The Dream: Random Sex with a Stranger. So your promiscuous side came out to play with a total stranger while you were sound asleep and you’re wondering what this risky business was all about.
Hey there, fellow outies and innies (I say, as I pen this at my office under the rotisserie chicken glow of florescent light). Thank *Kier* Severance is back for season two! The AppleTV+ hit left ...
This class is named after the prototype and brightest example, RR Lyrae. They are pulsating horizontal branch stars of spectral class A or F, with a mass of around half the Sun 's. They are thought to have shed mass during the red-giant branch phase, and were once stars at around 0.8 solar masses.
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