Examples of using Supernova in English and their translations into Bengali
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The supernova will come and will destroy everything.
However, not every star will become a supernova.
It is mainly a supernova or a type of astral explosion.
In 2015 Dr. Mullerreceived the Breakthrough Prize in Fundamental Physics for the Supernova Cosmology project.
Supernova CG and Epoch| Neutron cards with new release Etere 26.3.
However, another team researcher analyzed that data,saying that a star exploded or the creation of The Cowe from Supernova.
Roughly one supernova explodes in a galaxy every one hundred years.
However, another team researcher analyzed that data,saying that a star exploded or the creation of The Cowe from Supernova.
In this supernova explosion… a single star outshines the rest of its galaxy.
The flux of gamma rays and x-rays indicates that the supernova was relatively close to us(perhaps 200 parsecs or 600 ly).
One supernova can create more energy than the Sun will throughout its entire lifetime.
Eta Carinae is nearing the end of its life andwill explode as a supernova probably some time in the next million years or so.
One supernova can create more energy than the Sun will throughout its entire lifetime.
The vast majority of the neutrinos streaming through the Earth originate from the Sun,but 24 neutrinos were also detected from supernova 1987A.
Cool Fact: One supernova can create more energy than the Sun will throughout its entire lifetime.
Along with Carl Pennypacker, Muller started The Berkeley Real Time Supernova Search, which became The Berkeley Automated Supernova Search.
In 1998 a supernova remnant, RX J0852.0-4622, was found in front(apparently) of the larger Vela Supernova Remnant.
Closely orbiting binary stars can follow more complex evolutionary paths, such as mass transfer onto a whitedwarf companion that can potentially cause a supernova.
The most recent supernova to be seen in the Milky Way galaxy was SN 1604, which was observed October 9, 1604.
The carbon must then be scattered through space in a supernova explosion, and eventually condense as part of a planet in a new-generation solar system.
Supernova SN 1054 was another widely observed event, with Arab, Chinese, and Japanese astronomers recording the star's appearance in 1054 CE.
The brightest stellar event inrecorded history was the SN 1006 supernova, which was observed in 1006 and written about by the Egyptian astronomer Ali ibn Ridwan and several Chinese astronomers.
The stellar wind and supernova explosions from these stars eventually cause the cloud to disperse, often leaving behind one or more young open clusters of stars.
One of the many amateur astronomers looking for supernovae, Caroline Moore, a member of the Puckett Observatory Supernova Search Team, found supernova SN 2008ha late November 2008.
The SN 1006 supernova, the brightest apparent magnitude stellar event in recorded history, was observed by the Egyptian Arabic astronomer Ali ibn Ridwan and the Chinese astronomers in 1006.
In particular, in 1998 two groups of cosmologists, the Supernova Cosmology Project and the High-Z Supernova Search Team, independently came to this conclusion observing the redshift of supernovae.
In 1998 two groups, the Supernova Cosmology Project and High-Z Supernova Search, were looking at the same phenomenon, redshifts of Type Ia supernovae.
In this period a supernova can emit as much energy as the Sun might over its entire lifetime.
There are fewer records of supernova SN 1181, which occurred in the constellation Cassiopeia just over a century after SN 1054.