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Beta Carinae is the second-brightest star in the southern constellation of Carina. It has the official name Miaplacidus; [14] Beta Carinae is the star's Bayer designation, which is Latinised from β Carinae and abbreviated Beta Car or β Car. With apparent magnitude of 1.69, [3] it is one of the brightest stars in the night sky.
IC 2448 is an elliptical planetary nebula in the constellation of Carina. It was discovered in 1898 by Williamina Fleming . [ 3 ] It lies near the bright star Beta Carinae , and the southern Carina can be explored in the months of autumn in the southern hemisphere .
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It lies near the Carina Nebula and at a comparable distance. A 5th magnitude star, it is visible to the naked eye under good observing conditions. A light curve for V371 Carinae, plotted from Hipparcos data [9] In 1977, Christiaan Sterken announced his discovery that HD 96919 is a variable star. [10] It was given its variable star designation ...
Luminous blue variable stars can undergo "giant outbursts" with dramatically increased mass loss and luminosity. η Carinae is the prototypical example, [20] with P Cygni showing one or more similar outbursts 300–400 years ago, [21] but dozens have now been catalogued in external galaxies.
How To Use Beau Monde. Similar to my husband’s grandmother’s application of the seasoning, many commenters mentioned using the blend in a vintage recipe called Beau Monde Dip, which Long ...
Intramuscular fat, contained within muscle tissue, increases the risk of serious heart disease, regardless of other risk factors, a new study suggests.
A U band light curve for V415 Carinae, adapted from Schröder and Hünsch (1992) [8] HR 2554 has two components in orbit around each other, making it a binary star. The semi-major axis of the secondary's orbit is 2.17 arcseconds. Thomas B. Ake and Sidney B. Parsons discovered that HR 2554 is a variable star, in 1986. [9]