Ancient Egypt Gods
Orion’s Belt or the Belt of Orion is an asterism in the constellation Orion. The asterism consists of three bright stars Alnitak, Alnilam, and Mintaka
The asterism is sometimes more commonly known as the Three Kings or Three sisters. The most famous Western culture reference with Orion’s belt is the Three Kings. It is a direct reference to the biblical tale of the three kings who offered gifts to the baby Christ.
This asterism, which is among the brightest and most prominent asterisms in the winter sky, is often used to find the Orion constellation. In regards to the three stars, the names of the outer two both mean “belt” in Arabic.
Alnilam however, comes from an Arabic word that means “string of pearls.” This is actually the name of the whole asterism in Arabic. In Chinese mythology, they were known as The Weighing Beam.
Alnitak is the second closest star to us from Orion’s belt at a distance of 1.260 light-years. It isn’t actually a single star, but rather a triple star system.
It is situated in the eastern end of Orion’s belt. Alnitak B is a 4th-magnitude B-type star which orbits Alnitak A once every 1.500 years. The primary star, Alnitak A is actually a blue supergiant of spectral type 09.7 lbe. It has an apparent magnitude of 2.0.
Alnitak A is around 28 times as massive as the Sun. Its diameter is 20 times greater and it is the brightest star of class O in the night sky. It is 250.000 times brighter than our sun with surface temperatures of around 29.500 K. It is believed that the star is around 6.4 million years old.
Alnitak Ab is around 14 times more massive than our sun. It is a blue dwarf of spectral type O9V, and it has an apparent magnitude of 4. It has around 7 times the sun’s mass and it is 32.000 times more bright. Its surface temperatures are around 29.000 K.
This star is much older than the primary star, at around 7.2 million years old. Not much is known about the third star Alnitak B, with the exception that it is also older, at around 7 million years old. It has a radial velocity of around 350 km / 217 mi per second.
Alnilam is a supergiant at around 2.000 light-years away from Earth, located in the middle of the belt.
It has a magnitude of 1.70 and it is the 29th-brightest star in the night sky and the fourth-brightest in Orion. Alnilam is around 375.000 times brighter than our sun while other estimates place it at around 832.000 times more brighter.
This giant is between 30 to 60 times more massive than our sun and has an estimated average surface temperature of around 27.500 K. It is a young star at around 5.7 million years old. When it comes to its radius, it has about 32.4 solar radii.
Mintaka is a multiple star system at around 1.200 light-years away from Earth. It is located at the western end of Orion’s belt.
The star is around 190.000 times more luminous than the Sun. The primary star, Mintaka Aa1, is 24 times more massive than our sun. It has surface average temperatures of around 29.000 K. Its radius is around 16.5 times that of the sun.
The primary component is itself a triple star system consisting of a class 09.5 bright giant and a class B main-sequence star. They orbit around each other once every 5.73 days.
Curiously, the ages of all the stars of the Mintaka system are currently unknown. Mintaka Aa2 is 8.4 times as massive as the sun and has around 6.5 solar radii. It is 16.000 times brighter than our sun and its average surface temperatures are around 25.600 K. The third star, Mintaka Ab is 22.5 times more massive than our sun. It has around 10.4 solar radii and it is 63.000 times brighter. The average surface temperatures are estimated to be around 28.400 K. The last two components of the Mintaka star system are much smaller.
The fourth, Mintaka B, has only 0.77 solar radii, 0.4 the sun’s luminosity and its surface temperatures are around 5.324 K, similar to the sun’s. The fifth component, HD 36485, is around 9 times more massive than the sun with around 5.7 solar radii. It is 3.300 times brighter, and its average surface temperature is around 18.400 K.
It is speculated that the three stars which form Orion’s belt, probably formed about the same time some ten million years ago from the molecular clouds in Orion.
It is estimated that Alnilam will turn into a red supergiant and explode within the next million years. The supernova explosion will be visible from Earth. However, the three stars will continue to remain Orion’s belt for many years to come.
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