Messier 7, also known as the Ptolemy Cluster, or NGC 6475, is an open cluster, being the southernmost Messier object. Epsilon Scorpii, also known as Larawag, is the fifth brightest star in Scorpius, located at around 63.7 light-years away from us.

Most of the stars here are hot, blue B-type stars, yet the brightest member is an orange K-type giant star, BM Scorpii. The primary star, Shaula A, has around 1,450% of our Sun’s mass, 880% of its radius, and it is 36,500 times brighter than our Sun. It is actually a triple-star system located some 500 light-years away.
The Butterfly Nebula, also known as NGC 6302, the Bug Nebula, or Caldwell 69, is a bipolar planetary nebula located at around 3,400 light-years away. Pi Scorpii is a blue-white star at 590 light-years from Earth, who is part of a triple system, is a star family, he is married to Pi Scorpii Ab, and the two have a son, Pi Scorpii B, who is an unknown star. Antares is actually a binary star, with its two components being the red supergiant star Antares A, and a hot main-sequence star, Antares B. Antares A has around 1,100% of our Sun’s mass, 6,800% of its radius, it is 75,900 times brighter than our Sun. Pi Scorpii A has an estimated temperature of around 25,000 Kelvins and gives off a luminosity of 21,900 suns. Considerando sua distância de 459 anos-luz em relação à Terra, sua magnitude absoluta é igual a −2.85. It is situated in a field of the Milky Way that is rich in nebulae, and it can be observed through modest telescopes. Sua magnitude aparente é igual a 2.89. There are only four Messier objects in the constellation of Scorpius, the open clusters Messier 6, and Messier 7, and the globular clusters Messier 4 and Messier 80. It is a minor meteor shower with around 3 meteors per hour at its peak. Messier 6 has a radius of 6 light-years, it is 94.2 million years old, and contains 120 stars, raging around magnitude 15.1. It has an apparent magnitude of 3.33, being among the brightest of the southern stars of Scorpius.

It is among the most prominent sites of massive star formation in the Milky Way.

Shaula, designated as Lambda Scorpii, is the second-brightest star in the constellation of Scorpius, and the 24th brightest star in the night sky.
Wray 17-96 is one of the most luminous stars in the galaxy, being 1,800,000 times brighter than our Sun. This open cluster has an apparent magnitude of 3.3, and it has a radius of 25 light-years.

Libra was known as the Claws of the Scorpion in Babylonia. A spectrum of Pi Scorpii has been recorded from 1003 to 1172 A with a maximum SNR of about 20 and a velocity resolution of 2.4 km/s. Lesath has around 1,140% of our Sun’s mass, 610% of its radius, and it is 7,381 times brighter than our Sun.

In some old descriptions, the constellation of Libra is treated as the Scorpion’s celestial claws. Messier 4 is a loosely concentrated cluster of class IX and measures around 75 light-years across, and it is around 12.2 billion years old. Scorpius X-1 is 60,000 times brighter than our Sun, having around 140% of our Sun’s mass. Shaula has an apparent magnitude of 1.62., and it is actually a triple star system, composed out of two B-type stars and a pre-main-sequence star.


Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever. This star marks one of the claws of the scorpion in the constellation Scorpius.

Viewed in visible light, this portion of the sky seems somewhat unremarkable. Both of its members are hot, B-type main-sequence stars that regularly eclipse each other. Messier 80 has an apparent magnitude of +7.87 and has a radius of around 48 light-years. The brightest star in Scorpius is the red supergiant Antares, which has an apparent magnitude of 0.6, which varies up to 1.6 and +5.5. It has an apparent magnitude of +5.9.

The constellation of Scorpius hosts 4 Messier objects, they are the open clusters Messier 6, and Messier 7, and the globular clusters Messier 4 and Messier 80. With an average apparent magnitude of 0.96, it is the brightest star in … The primary star, Girtab A, is also a variable Beta Cephei star.

The primary star A, forms an eclipsing binary event of the Beta Lyrae type. Dense Clumps of Ionized Gas near pi Scorpii, as Revealed by the Fine-Structure Excitation of N II Bertoldi, Frank; Jenkins, Edward B. Abstract. The best time to observe them is during the month of July. Scorpius pre-dates the Greeks, being an ancient constellation. Some other interesting deep-sky objects in Scorpius include the NGC 6231 open cluster, the planetary nebula 6302, or the Cat’s Paw Nebula. Antares is the brightest, most massive, and most evolved star of the nearest OB association, the Scorpius-Centaurus Association. Antares is a red supergiant star and a slow irregular variable star that ranges in brightness from magnitude +0.6 to +1.6. Pi Scorpii (π Scorpii, förkortat Pi Sco, π Sco), som är stjärnans Bayer-beteckning, är en trippelstjärna [12] i den västra delen av stjärnbilden Skorpionen.Den har en genomsnittlig skenbar magnitud på +2,89 [2] och är synlig för blotta ögat. It has an apparent magnitude of 2.70.

Poor Relationships The secondary star, SW, has around 6.600% of our Sun’s mass, 1,700% of its radius, and it is 646,000 times brighter than our Sun. Currently, around 14 stars in Scorpius have been confirmed to host planets. If you picture the "thumb" and "forefinger" making a circle, it is as though you are seeing a celestial "okay" sign. July 2, 2020 by admin. The Butterfly Nebula has a radius of around 1.5 light-years. Scorpius is one of the twelve zodiac constellations, located in the southern celestial hemisphere. How to choose your telescope magnification? The Babylonians called Scorpius MUL.GIR.TAB – the creature with the burning sting.

This nebula is also known as the Lobster Nebula or the Madokami Nebula.

Zeta1 Scorpii is a B-type hypergiant located at around 2,600 light-years away from us. Some people see this nebula as an arm and hand emerging from the cosmos. Eta Scorpii has around 175% of our Sun’s mass, 1,770% of its radius, and it is a fast-spinning star, having a rotational velocity of around 150 km / 93.2 mi per second.

The Alpha Scorpiids occur between 21 April and May 26th, peaking on May 15th every year.

It has an apparent magnitude of 11.00. This star is hotter than our Sun as well, having temperatures of around 23,400 K, and it is also spinning fast, having a rotational velocity of 105 km / 65.2 mi per second.

This cluster is around 200 million years old. Much like gazing at Earth-bound clouds, it is fun to use your imagination when looking at images of nebulae.

After Zeus raised Orion and the scorpion in the sky, the former hunts every winter but flees every summer when the scorpion returns. https://simple-cosmos-official.fandom.com/wiki/Pi_Scorpii?oldid=7464.

Blue represents infrared radiation at 3.4 microns, while green represents light with a wavelength of 4.6 microns. xmlns:xsl='http://www.w3.org/1999/XSL/Transform'">. The bright star on the right with the greenish haze is Pi Scorpii. This star is quite young, being around 20 million years old. Currently, around 14 stars in Scorpius have been confirmed to host planets.

It has an apparent magnitude of 1.87, being the 39th brightest star in the night sky. Perhaps a cross-species celestial handshake is imminent?

There is also an exoplanet in this system which orbits the stars. There are two meteor showers associated with the constellation of Scorpius, the Alpha Scorpiids, and the Omega Scorpiids. The Javanese people of Indonesia called Scorpius the Banyakangrem – the brooded swan – or Kalapa Doyong – leaning coconut tree – due to its shape. PI SCO (Pi Scorpii).

It has an apparent magnitude of 7, and the structure in this nebula is among the most complex ever observed. It contains many unique and interesting stars. It is also a fast-spinning star having a rotational velocity of around 125 km / 77.6 mi per second. Type of Star


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