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supernova and 1572
The astronomer Tycho Brahe observed the supernova SN 1572 in the constellation Cassiopeia, and described it in his book De stella nova ( Latin for " concerning the new star "), giving rise to the name nova.
** A supernova, now designated as SN 1572, is first observed in the constellation Cassiopeia by Cornelius Gemma.
Multiwavelength composite image of the remnant of Tycho's supernova, SN 1572.
Other well-known supernova remnants include the Crab Nebula, Tycho, the remnant of SN 1572, named after Tycho Brahe who recorded the brightness of its original explosion, and Kepler, the remnant of SN 1604, named after Johannes Kepler.
A composite image of the remnants of the SN 1572 supernova
An example of such an event is the supernova SN 1572, which was observed by Tycho Brahe.
* That he observed the location of Tycho Brahe's supernova of 1572 and found a star there which he estimated to be " somewhat dimmer than Jupiter's third moon.
It argued against the certainty of the astronomical theory of stellar parallax, and the terrestrial origin of the " comet of 1573 " ( i. e. the supernova SN 1572 ).
* SN 1572, a supernova remnant, often called Tycho's supernova
Four historical supernovae are known simply by the year they occurred ( SN 1006, 1054, 1572 Nova, and 1604 Star ); starting with 1885, the letters are used, even if there was only one supernova detected that year ( e. g. SN 1885A, 1907A, etc.
* November 9-A supernova, now designated as SN 1572, is first observed in the constellation Cassiopeia by Cornelius Gemma.
Thomas attempted to determine the parallax of the 1572 supernova observed by Tycho Brahe, and concluded it had to be beyond the orbit of the Moon.
He published his studies of a supernova in the constellation Cassiopeia in 1572.
" Al Aaraaf " is the longest poem Poe wrote and was inspired by Tycho Brahe's discovery of a supernova back in 1572 which was visible for about seventeen months.
SN 1572 ( Tycho's Supernova, Tycho's Nova ), " B Cassiopeiae " ( B Cas ), or 3C 10 was a supernova of Type Ia in the constellation Cassiopeia, one of about eight supernovae visible to the naked eye in historical records.
Star map of the constellation Cassiopeia showing the position ( labelled I ) of the supernova of 1572 ; from Tycho Brahe's De nova ... stella
The appearance of the Milky Way supernova of 1572 was perhaps one of the two or three most important events in the history of astronomy.
But Tycho was not even close to being the first to observe the 1572 supernova, although he was apparently the most accurate observer of the object ( though not by much over some of his European colleagues like Wolfgang Schuler, Thomas Digges, John Dee and Francesco Maurolico ).

supernova and is
By measuring the velocities of pulsars, it is possible to put a limit on the asymmetry of supernova explosions.
The abundance of elements in the Solar System is in keeping with their origin from nucleosynthesis in the Big Bang and a number of progenitor supernova stars.
In supernova explosions, calcium is formed from the reaction of carbon with various numbers of alpha particles ( helium nuclei ), until the most common calcium isotope ( containing 10 helium nuclei ) has been synthesized.
* 1054 – A supernova is seen by Chinese, Arab, and possibly Amerindian observers near the star Zeta Tauri.
The historic supernova SN 1006 is described by various sources as appearing on April 30 to May 1, 1006, in the constellation of Lupus.
The relative abundance of magnesium is related to the fact that it is easily built up in supernova stars from a sequential addition of three helium nuclei to carbon ( which in turn is made from three helium nuclei ).
Manganese is part of the iron group of elements, which are thought to be synthesized in large stars shortly before the supernova explosion.
On Earth, such native nickel is always found in combination with iron, a reflection of those elements ' origin as major end products of supernova nucleosynthesis.
Nickel-78's half-life was recently measured to be 110 milliseconds and is believed to be an important isotope involved in supernova nucleosynthesis of elements heavier than iron.
The r process is thought to occur in supernova explosions because the conditions of high temperature, high neutron flux and ejected matter are present.
The supernova event was recorded in the year 1054 and is labelled SN 1054.
Although much of the optical and X-ray emission from supernova remnants originates from ionized gas, a great amount of the radio emission is a form of non-thermal emission called synchrotron emission.
A neutron star is a type of stellar remnant that can result from the gravitational collapse of a massive star during a Type II, Type Ib or Type Ic supernova event.
As the core of a massive star is compressed during a supernova, and collapses into a neutron star, it retains most of its angular momentum.
A fraction of the mass of a star that collapses to form a neutron star is released in the supernova explosion from which it forms ( from the law of mass-energy equivalence, ).
It is thought to be at the brink of becoming a type-1a supernova.
Astronomers speculate that this phenomenon is caused by the shock wave from a supernova.
An even more speculative hypothesis is that intense radiation from a nearby supernova was responsible for the extinctions.
In Cryptic Studios online role-playing game, Star Trek: Online, Janeway is briefly mentioned in the background, exploring the Hobus system after the supernova that was the catalyst for the events of the 2009 Star Trek movie.
During the events of the comic book mini-series Star Trek: Countdown ( which serves as the canonical prequel to the 2009 Star Trek film ), Geordi ( now a commander ) is reunited with Data and Picard during an effort to stop a massive supernova that threatens all of existence.
According to the 2009 film Star Trek and the prequel comic series Star Trek: Countdown, Romulus ( and presumably Remus ) is destroyed in 2387 by a star going supernova.
The problems of the Hobus supernova being so devastating to other solar systems is addressed in the computer game Star Trek Online, by declaring the blast to have " traveled through subspace ".
A supernova ( abbreviated SN, plural SNe after supernovae ) is a stellar explosion that is more energetic than a nova.

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