Cyclocardia Bailyi
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Cyclocardia Bailyi
''Cyclocardia'' is a genus of molluscs in the family Carditidae. The related genus ''Vimentum'' is sometimes included here. Species * ''Cyclocardia astartoides'' (Martens, 1878) *†''Cyclocardia awamoensis'' (Harris, 1897) * ''Cyclocardia bailyi'' (J. Q. Burch, 1944) * ''Cyclocardia barbarensis'' (Stearns, 1890) * ''Cyclocardia beebei'' (Hertlein, 1958) * ''Cyclocardia borealis'' – northern cardita *†''Cyclocardia christiei'' (Marwick, 1929) * ''Cyclocardia compressa'' (Reeve, 1843) * ''Cyclocardia congelascens'' (Melvill & Standen, 1912) * ''Cyclocardia crassidens'' (Broderip & Sowerby I, 1829) * ''Cyclocardia crebricostata'' (A. Krause, 1885) * ''Cyclocardia dalek'' Pérez & Del Río, 2017 * ''Cyclocardia gouldii'' (Dall, 1903) *†''Cyclocardia granulata'' (Say, 1824) * ''Cyclocardia incisa'' (Dall, 1903) * ''Cyclocardia isaotakii'' (Tiba, 1972) *†''Cyclocardia magna'' Quilty, Darragh, Gallagher & Harding, 2016 *†''Cyclocardia marama'' (P. A. Maxwell, 1969) * ''Cy ...
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Arcturus (isopod)
, - bgcolor="#FFFAFA" , Note (category: variability): , , H and K emission vary. Arcturus is a red giant star in the northern constellation of Boötes, and the brightest star in the constellation. It has the Bayer designation α Boötis, which is Latinized to Alpha Boötis and abbreviated Alf Boo or α Boo. With an apparent visual magnitude of −0.05, it is the fourth-brightest star in the night sky and the brightest in the northern celestial hemisphere. Arcturus forms one corner of the Spring Triangle asterism. Located relatively close at 36.7 light-years from the Sun, Arcturus is a red giant of spectral type K1.5III—an aging star around 7.1 billion years old that has used up its core hydrogen and evolved off the main sequence. It is about the same mass as the Sun, but has expanded to 25 times its size (around 35 million kilometers) and is around 170 times as luminous. Nomenclature The traditional name ''Arcturus'' is Latinised from the ancient Greek ''Ἀ ...
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