- published: 02 Aug 2016
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SN 1987A was a supernova in the outskirts of the Tarantula Nebula in the Large Magellanic Cloud (a nearby dwarf galaxy). It occurred approximately 51.4 kiloparsecs from Earth, approximately 168,000 light-years, close enough that it was visible to the naked eye. It could be seen from the Southern Hemisphere. It was the closest observed supernova since SN 1604, which occurred in the Milky Way itself. The light from the new supernova reached Earth on February 23, 1987. As it was the first supernova discovered in 1987, it was labeled “1987A”. Its brightness peaked in May with an apparent magnitude of about 3 and slowly declined in the following months. It was the first opportunity for modern astronomers to see a supernova up close and observations have provided much insight into core-collapse supernovae. Of special importance, SN1987A provided the first chance to confirm by direct observation the radioactive source of the energy for visible light emissions by detection of predicted gamma-ray line radiation from two of its abundant radioactive nuclei, 56Co and 57Co. This proved the radioactive nature of the long-duration post-explosion glow of supernovae.
Trousers (pants in North America) are an item of clothing worn from the waist to the ankles, covering both legs separately (rather than with cloth extending across both legs as in robes, skirts, and dresses).
In the UK the word "pants" generally means underwear and not trousers.Shorts are similar to trousers, but with legs that come down only to around the area of the knee, higher or lower depending on the style of the garment. To distinguish them from shorts, trousers may be called "long trousers" in certain contexts such as school uniform, where tailored shorts may be called "short trousers", especially in the UK.
In most of the Western world, trousers have been worn since ancient times and throughout the Medieval period, becoming the most common form of lower-body clothing for adult males in the modern world, although shorts are also widely worn, and kilts and other garments may be worn in various regions and cultures. Breeches were worn instead of trousers in early modern Europe by some men in higher classes of society. Since the mid-20th century, trousers have increasingly been worn by women as well. Jeans, made of denim, are a form of trousers for casual wear, now widely worn all over the world by both sexes. Shorts are often preferred in hot weather or for some sports and also often by children and teenagers. Trousers are worn on the hips or waist and may be held up by their own fastenings, a belt or suspenders (braces). Leggings are form-fitting trousers, of a clingy material, often knitted cotton and spandex (elastane).
The Large Magellanic Cloud (LMC) is a nearby galaxy, and a satellite of the Milky Way. At a distance of 50 kiloparsecs (≈163,000 light-years), the LMC is the third closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (~ 16 kiloparsecs) and the putative Canis Major Dwarf Galaxy (~ 12.9 kiloparsecs, though its status as a galaxy is under dispute) lying closer to the center of the Milky Way. The LMC has a diameter of about 14,000 light-years (~ 4.3 kpc) and a mass of approximately 10 billion Sun masses (1010solar masses), making it roughly 1/100 as massive as the Milky Way. The LMC is the fourth largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33).
In the past, the LMC was often considered an irregular type galaxy. However, it is now recognized as a disrupted barred spiral galaxy. The NASA Extragalactic Database, however, still lists the Hubble sequence type as Irr/SB(s)m). In reality, the LMC contains a very prominent bar in its center, suggesting that it may have previously been a standard barred spiral galaxy before being disrupted, likely by the gravitational tug of the Milky Way, resulting in the disruption of its spiral arms. The LMC's present irregular appearance is likely the result of tidal interactions with both the Milky Way and the Small Magellanic Cloud (SMC).
The Milky Way is the galaxy that contains our Solar System. Its name "milky" is derived from its appearance as a dim glowing band arching across the night sky whose individual stars cannot be distinguished by the naked eye. The term "Milky Way" is a translation of the Latin via lactea, from the Greek γαλαξίας κύκλος (galaxías kýklos, "milky circle"). From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from within. Galileo Galilei first resolved the band of light into individual stars with his telescope in 1610. Until the early 1920s, most astronomers thought that the Milky Way contained all the stars in the Universe. Following the 1920 Great Debate between the astronomers Harlow Shapley and Heber Curtis, observations by Edwin Hubble showed that the Milky Way is just one of many galaxies—now estimated to number as many as 200 billion galaxies in the observable universe.
The Milky Way is a barred spiral galaxy that has a diameter usually considered to be about 100,000–120,000 light-years but may be 150,000–180,000 light-years. The Milky Way is estimated to contain 100–400 billion stars, although this number may be as high as one trillion. There are probably at least 100 billion planets in the Milky Way. The Solar System is located within the disk, about 27,000 light-years from the Galactic Center, on the inner edge of one of the spiral-shaped concentrations of gas and dust called the Orion Arm. The stars in the inner ≈10,000 light-years form a bulge and one or more bars that radiate from the bulge. The very center is marked by an intense radio source, named Sagittarius A*, which is likely to be a supermassive black hole.
Brightest Supernova (SN 1987A) Ever Seen in the Large Magellanic Cloud
Zoom on SN1987A
Supernova II (SN 1987A) 1988 NASA JPL Jet Propulsion Laboratory
SN 1987A
SN 1987A
SN 1987A, animation
Zoom on supernova SN1987A
Hubble's view of Supernova 1987A over time
Supernona SN1987a rendered with glnemo2
SN 1987A 1994-2006 - Annotated
SN 1987A Brightest Supernova Ever Seen in the Large Magellanic Cloud SN 1987A was the brightest exploding star seen in 400 years when astronomers spotted it on Feb. 23, 1987. The violent death of a star 20 times more massive than the Sun, called a supernova, created this stellar drama. The star actually exploded about 160,000 years ago, but it has taken that long for its light to reach Earth. The supernova resides in the Large Magellanic Cloud, a nearby small galaxy that is a satellite of our Milky Way galaxy. The ring, about a light-year across, already existed when the star exploded. This is a rare opportunity for astronomers to see exactly how a supernova explosion is transformed into a supernova remnant, the glowing, expanding gaseous remains of a supernova blast. The elongated and ...
Astronomers using ESO's Very Large Telescope have for the first time obtained a three dimensional view of the distribution of the innermost material expelled by a recently exploded star, known as Supernova 1987A (or SN 1987A). The original blast was not only powerful, according to the new results. It was also more concentrated in one particular direction. This is a strong indication that the supernova must have been very turbulent, supporting the most recent computer models. SN 1987A lies in the Large Magellanic Cloud, 165 000 light-years from Earth. This video zooms into images of SN 1987A as seen with ESO telescopes, and finally fades into an artist's impression that shows the different elements present in SN 1987A: two outer rings, one inner ring and the deformed, innermost expelled ma...
more at http://scitech.quickfound.net/astro/astronomy_news_and_links.html "Describes the recent discovery of the supernova SN 1987A on February 23, 1987. NASA scientists explain how natural nucleosynthesis (formation of heavy elements) occurs when a supernova is formed and how studying the death of stars will help explain the origin of the universe." Public domain film from NASA, slightly cropped to remove uneven edges, with the aspect ratio corrected, and one-pass color correction & mild video noise reduction applied. The soundtrack was also processed with volume normalization, noise reduction, clipping reduction, and/or equalization (the resulting sound, though not perfect, is far less noisy than the original). http://creativecommons.org/licenses/by-sa/3.0/ https://en.wikipedia.org/wi...
Discovered in 1987, Supernova 1987A is the closest exploding star to Earth to be detected since 1604 and it resides in the nearby Large Magellanic Cloud, a dwarf galaxy adjacent to our own Milky Way Galaxy.
The unique supernova SN 1987A has been a bonanza for astrophysicists. It provided several observational firsts, like the detection of neutrinos from an exploding star, the observation of the progenitor star on archival photographic plates, the signatures of a non-spherical explosion, the direct observation of the radioactive elements produced during the blast, observation of the formation of dust in the supernova, as well as the detection of circumstellar and interstellar material. The footage available include images of the supernova taken in the past, as well as the most recent one obtained with ESOs Very Large Telescope, and images of the La Silla and Paranal Observatories. A breathtaking sequence that zooms-in from the Large Magellanic Cloud into the supernova is also available.
The animation illustrates the events following the supernova 1987A outburst. The blue ring is previously observed material ejected from the star thousands of years ago. The expanding orange and yellow shell is multimillion degree, X-ray emitting gas produced by the explosion. Portions of the blue ring light up when struck by the X-ray shell. Animation: NASA/CXC/D.Berry
Astronomers using ESO's Very Large Telescope have for the first time obtained a three dimensional view of the distribution of the innermost material expelled by a recently exploded star, known as Supernova 1987A (or SN 1987A). The original blast was not only powerful, according to the new results. It was also more concentrated in one particular direction. This is a strong indication that the supernova must have been very turbulent, supporting the most recent computer models. SN 1987A lies in the Large Magellanic Cloud, 165 000 light-years from Earth. This video zooms into images of SN 1987A as seen with ESO telescopes, and finally fades into an artist's impression that shows the different elements present in SN 1987A: two outer rings, one inner ring and the deformed, innermost expelled ma...
Time-series images made by cameras onboard the Hubble Space Telescope show the evolution of the inner remnant of Supernova 1987A. Video courtesy of Peter Challis; NASA
Movie of supernova 1987A rendered with glnemo2 visualization program (see http://projets.lam.fr/projects/glnemo2). Simulation has been run by Thomas Morris and Philipp Podsiadlowski. The relevant paper is: "The triple-ring nebula around SN 1987A: fingerprint of a binary merger." Morris, T., Podsiadlowski, Ph., 2007, Science, 315, 1103
http://www.astropage.eu/index_news.php?id=798 Astro-Bild der Woche: Der Supernova-Überrest SN 1987A A time-lapse sequence of 12 years of Hubble observing SN 1987A shows the onrushing stellar shock wave from the stellar explosion as it is slamming into, heating up, and illuminating the inner regions of the narrow ring surrounding the doomed star. Credit: NASA, ESA, and G. Bacon (STScI)