Search results
Results from the WOW.Com Content Network
TON 618 (abbreviation of Tonantzintla 618) is a hyperluminous, broad-absorption-line, radio-loud quasar, and Lyman-alpha blob [2] located near the border of the constellations Canes Venatici and Coma Berenices, with the projected comoving distance of approximately 18.2 billion light-years from Earth.
Baker–Miller Pink, also known as P-618, Schauss pink, or Drunk-Tank Pink is a tone of pink which has been observed to temporarily reduce hostile, violent or aggressive behavior. [1] It was originally created by mixing white indoor latex paint with red trim semi-gloss outdoor paint in a 1:8 ratio by volume.
If this object were 10 parsecs away from Earth it would appear nearly as bright in the sky as the Sun (apparent magnitude −26.744). This quasar's luminosity is, therefore, about 2 trillion (10 12) times that of the Sun, or about 100 times that of the total light of average large galaxies like our Milky Way. (Note that quasars often vary ...
Bright pink is a maximally saturated tone of pink that is another name for the color rose. In most Indo-European languages , the color that in English is called pink is called rosa ; therefore, the color that is called rose in English is called bright rosa in most European and Latin American countries (using whatever adjective in a particular ...
Size comparison of a hypothetical quasi-star to some of the largest known stars. A quasi-star rendered with Celestia. A quasi-star (also called black hole star) is a hypothetical type of extremely large and luminous star that may have existed early in the history of the Universe.
In 1960, a group of astronomers working at the Radcliffe Observatory in Pretoria made systematic measurements of the brightness and spectra of bright stars in the Large Magellanic Cloud (LMC). Among the objects cataloged was RMC 136 (Radcliffe observatory Magellanic Cloud catalog number 136), the central "star" of the Tarantula Nebula , which ...
In daytime, sodium and red oxygen emissions are dominant and roughly 1,000 times as bright as nighttime emissions because in daytime, the upper atmosphere is fully exposed to solar UV radiation. The effect is however not noticeable to the human eye, since the glare of directly scattered sunlight outshines and obscures it.
12.618 [6] Characteristics Spectral type: A3 V / K5Vp / M4V [6] [7] ... Researchers find that bright nearby double star Fomalhaut is actually a triple ...