It has an apparent magnitude of 7.87 and is approximately 32,600 light-years distant from the Sun.M80 is one of the most densely populated clusters in our galaxy.
It got the name War and Peace Nebula because, when observed in infrared, the nebula’s western part resembles a dove, while the eastern part resembles a skull.
Agreement It is 170 more luminous than the Sun and has an orbital period estimated at 878 years.Antares marks the heart of the scorpion, which is also its alternative name. It’s time to aim your telescope at NGC 6302, a very curious planetary nebula located around three fingerwidths west of Lambda Scorpii: it is better known as … Sometimes the star is also known as Iclarcrau or Iclarkrav.This star is Scorpius’ most famous and brightest star. It has a companion star, Antares B, about 529 astronomical units (AU) away.Antares B has the stellar classification B2.5 and an apparent magnitude of 5.5. It has about 0.64 solar masses and is enveloped in a very dense equatorial disc of dust and gas.NGC 6357 is a diffuse nebula in Scorpius. Scorpius is the southernmost constellation of the Zodiac.The Sumerians called it GIR-TAB, or “the scorpion”. Thus the ionization of this nebula may be the result of both collisional (the high-ionization lines) and photoionization (the traditional nebular lines). 12" f/15 Cassegrain 18mm no filter pretty bright, pretty small, very much elongated 1.8X1 E-W.
Butterfly Nebula (Bug Nebula) – NGC 6302 (Caldwell 69) The Butterfly Nebula is a bipolar planetary nebula in Scorpius. Question: Consider the following statements regarding NGC- 6302: 1. The spectrum of NGC 6302 shows that its central star is one of the hottest stars in the galaxy. NGC 6302 lies within our Milky Way galaxy, roughly 3800 light-years away in the constellation of Scorpius. Its surface temperature is over 250,000 degrees Celsius.This means the star from which it formed must have been very large. The Bug Nebula has a high surface brightness. It seems more likely that the very high ionization lines are the result of shock ionization produced by strong winds from the central star. Lines of very highly ionized silicon recently discovered in the type I planetary nebula NGC 6302 implied a central star temperature of 450,000 K assuming that the high ionization lines were the result of photoionization. NGC 6302 5" f/8 QLD, Australia S=6 T=7 18mm pretty bright, small, elongated, not much at this aperture. Vnitřním uspořádáním se řadí mezi nejsložitější pozorované planetární mlhoviny.
It was discovered by the Swiss astronomer Philippe Loys de Chéseaux in 1746 and included in Messier’s catalog in 1764.M4 is easy to find in the sky, as it lies 1.3 degrees west of Antares. NGC 6744 is situated in the constellation of Pavo at a distance of about 25 million light-years.. Ptolemy believed the cluster to be a nebula.
It has an apparent magnitude of 7.1. 2. It lies in the third quadrant of the southern hemisphere (SQ3) and can be seen at latitudes between +40° and -90°.The neighboring constellations are Ara, Corona Australis, Libra, Lupus, Norma, Ophiuchus, and Sagittarius. M7, also known as the Ptolemy cluster, is an open cluster of about 80 stars.It is also known as the Ptolemy Cluster because it was the Greek astronomer Ptolemy who first recorded it in 130 AD. This is the highest central star temperature ever reported for a planetary nebula, and the effects of a luminous soft X-ray source on a surrounding nebula have never been examined. This image from the NASA/ESA Hubble Space Telescope depicts NGC 6302, commonly known as the Butterfly Nebula. It is believed to contain tens of thousands of stars.The nebula was discovered by the English astronomer John Herschel in 1837.The Butterfly Nebula is a bipolar planetary nebula in Scorpius. Simply look for a J-shaped pattern of stars between the constellations Libra (the scales) and Scorpius is one of the zodiac constellations, first cataloged by the Greek astronomer Ptolemy in the 2nd century.
Along with The bright stars in M4 are mostly hot, blue, class B stars, but the brightest one is a class K orange giant, BM Scorpii.The Butterfly Cluster has an apparent magnitude of 4.2 and is approximately 1,600 light-years distant from the Sun.Messier 7 is another open star cluster in Scorpius, located near the scorpion’s stinger. It has an apparent magnitude of 3.3 and can easily be seen with the naked eye.
However, we commonly associate this constellation with the Greek origins, associated with the story of Scorpius is the 33rd constellation in size, occupying an area of 497 square degrees. It is a planetary nebula, commonly known as butterfly nebula. The estimated age of the star system is about 10-13 million years.Lambda Scorpii’s traditional name, Shaula, comes from the Arabic al-šawlā´, which means “the raised (tail).”It was the first globular cluster discovered in which individual stars could be resolved. The age of the cluster is estimated to be around 200 million years.Messier 80 is a globular cluster discovered by Charles Messier in 1781. The Ptolemy Cluster contains about 80 stars, the brightest of which has a visual magnitude of 5.6.M7 is approximately 980 light-years distant from the solar system. It is one of the most structurally complex nebulae known.The central star, a white dwarf, has a surface temperature in excess of 200,000 K, which makes it one of the hottest stars in the galaxy.
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