Where is scorpio in relation to orion

When the world was new, the great hunter and giant Orion was feared by all the beasts. He slew many great beasts of the land and sea. None succeeded in staying his arrow. In a fit of arrogance, he proclaimed to the heavens that he would not rest until he succeeded in killing all the wild animals of the Earth. His insolence angered Gaia, goddess of the Earth and mother of the Titans. She sought the help of a lone scorpion and asked him to slay the giant. Initially, Orion was not afraid of the creature.

How could one so small ever dare to challenge his might? Each has at least 10 solar masses and both are expected to end their lives in massive Type II supernova events. Delta Scorpii has the stellar classification B0.

It has a visual magnitude of 2. The star has a class B companion orbiting it every 20 days, and another star in a very eccentric orbit that orbits the primary star every 10 years.

Sometimes the star is also known as Iclarcrau or Iclarkrav. Theta Scorpii is an evolved bright yellow giant star belonging to the spectral class F0 II. It has an apparent magnitude of 1.

The star has 5. It has a companion with an apparent magnitude of 5. The meaning of the name is unknown. The star has a radius almost 13 times that of the Sun. It is classified as a variable, as its brightness varies slightly, only by 0. Kappa Scorpii is a spectroscopic binary star, composed of two stars that cannot be resolved with a telescope. The stars have an orbital period of days. The combined spectrum of the Kappa Scorpii system has the stellar classification of B1.

The primary component in the system is classified as a Beta Cephei type variable, which is to say it is a star that exhibits variations in brightness as a result of pulsations of its surface. The star is 17 times more massive than the Sun and has almost 7 times the solar radius. The secondary component is also much larger than the Sun, has about 12 solar masses, and almost 6 times the solar radius.

Pi Scorpii is a triple star system with a combined visual magnitude of 2. It is approximately light years distant. The brightest components in the system form an eclipsing binary star classified as a Beta Lyrae type variable. Both stars are hot main sequence stars with the stellar classifications B1 V and B2 V. The distance between them is believed to be only around 15 solar radii. The third component in the system is a distant companion with a visual magnitude of The primary star is 21, times more luminous than the Sun and has about solar masses.

Nu Scorpii is another multiple star system in Scorpius, approximately light years distant from Earth. It is composed of two close groups of stars separated by 41 seconds of arc. The brighter group consists of B2 class subgiants and the fainter pair is comprised of class B8 and B0 main sequence dwarf stars. Xi Scorpii is another multiple star system in Scorpius. It consists of at least five stars forming two groups that are separated by 4. The brighter group consists of two yellow-white class F stars, a subgiant with a visual magnitude of 4.

The other group consists of two class K stars separated by The sixth component in the Xi Scorpii system is not confirmed to be gravitationally bound to the other stars. It is an 11th magnitude star. The Bayer designation Iota Scorpii is shared by two stars. Iota-1 Scorpii is an evolved star with the stellar classification F2 Ia, on the verge of becoming a supergiant. It is 12 times more massive than the Sun and about 35, times more luminous. It has a 10th magnitude companion at a separation of The star is sometimes known by its proper name, Apollyon.

Iota-2 Scorpii is a supergiant belonging to the spectral class A6Ib. It has an apparent magnitude of 4. The star has a distant 11th magnitude companion at a separation of Sigma Scorpii is a star system with a combined apparent magnitude of 2.

The brightest star in the system is a spectroscopic binary star, composed of two unresolved stars that orbit each other with a period of The primary star in the spectroscopic binary system is a giant of the spectral type B1 III. It is 18 times more massive than the Sun and has 12 times the solar radius. It is classified as a Beta Cephei type variable. The other component in the system is a main sequence star belonging to the spectral class B1 V. There is another star in the system orbiting the main pair at a separation of half an arc second.

At a separation of 20 seconds of arc, a class B9 dwarf with a visual magnitude of 8. Tau Scorpii is a hydrogen fusing dwarf star with a strong, complex magnetic field.

The star has the stellar classification B0. It is a hot star, with a mass 15 times that of the Sun and a radius more than six times solar. It has an apparent magnitude of 2. The star is about 18, times more luminous than the Sun. Tau Scorpii is a popular target for astronomers because it is so luminous and hot, and also because, as a result of its slow rotation, the star shows a very clear spectrum. U Scorpii is the fastest known nova and one of the 10 known recurring novae in the Milky Way galaxy.

The accumulated hydrogen ignites, causing nuclear fusion. U Scorpii normally has a visual magnitude of 18, but during outbursts it reaches magnitude 8. The last eruption was observed in and the next one is expected to occur in the year Upsilon Scorpii is a subgiant star belonging to the spectral class B2 IV. The star is about 11 times more massive and 12, times more luminous than the Sun, and has a radius 6.

Omega Scorpii is composed of two stars separated by 0. Omega-1 Scorpii is a blue-white dwarf belonging to the spectral class B1V.

It has an apparent magnitude of 3. The star used to be known as Gamma Telescopii. Eta Scorpii is a yellow-white subgiant star evolving into a giant. It has the stellar classification F5 IV and an apparent magnitude of 3. The star is It is believed to be around 1. It is 18 times more luminous than the Sun. It emits X-rays, and shows an enhanced abundance of barium in its spectrum. Rho Scorpii is another binary star in Scorpius. The contest was however such a lively one that it caught the attention of Zeus, the god of the sky and ruler of all Olympian gods, who then honoured Scorpius by raising it to the heavens.

Zeus obliged, placing them on opposite ends of the night sky; Scorpio can still be seen today, endlessly chasing Orion across the night sky. This myth serves as a reminder to mortal men to avoid arrogance and boastfulness and to care for all creatures, large and small. The constellation of Scorpius with the red supergiant Antares at the heart of the scorpion. Aside from the mythology, taking a closer look at Scorpius, there are some amazing facts from an astronomical point of view.

At the center of this 17 star constellation sits Antares, the heart of the scorpion, which is one of the largest know stars. This is a truly an enormous star and if placed at the center of our solar system, its surface would extend beyond the orbit of Mars.

The circumference of Antares measures in at a whopping times that of our Sun. It is a magnificent constellation and unlike many star constellations, is one that actually looks like its namesake! Filed under General Nature. Rob joined the Londolozi team at the start of Having grown up on a farm in the Cape and spending many holidays traveling Southern Africa he developed a love for the outdoors and an appreciation for the natural world.

After completing a Kirst Joscelyne Oct 25, Photography , The Week in Pictures. Sean Zeederberg Aug 20, 2 Photography , The Week in Pictures , Wildlife. Dean De La Rey Aug 13, 2 You must be logged in to post a comment. Thank you Rob I have always loved the stories of the night sky — you put it across beautifully! Interesting story, there is nothing more beautiful than a clear African night sky, Over the years have experienced many throughout Africa, thank you!

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