Orion (constellation)

from Wikipedia, the free encyclopedia

Orion constellation
Orion constellation map.png
Legend
Latin name Orion
Latin genitive Orionis
Abbreviation Ori
Right ascension 4432504 h 43 m 25 s to  06 h 25 m 47 s62547
declination 1894157−10 ° 58 ′ 43 ″ to  + 22 ° 52 ′ 35 ″2225235
surface 594.120 deg²
rank 26th
Completely visible 79.5 ° N to 67.6 ° S
Observation time for Central Europe winter
Number of stars brighter than 3 mag 8th
Brightest star (size) Rigel (0.12)
Meteor streams
Neighboring constellations
(
clockwise from north )
swell IAU ,
The constellation Orion as seen with the naked eye in the southeastern sky (taken in the Alps in 2003).
The constellation Orion as seen with the naked eye in the southeastern sky (taken in the Alps in 2003).

The Orion [ oʀiːɔn ] is a striking constellation of the winter sky on the celestial equator . It has two stars of the first magnitude , three stars of the second magnitude at approximately the same distance form the Orion belt .

description

The constellation lies on the celestial equator between the river Eridanus and the unicorn and can be seen in Central Europe from around August (morning sky) to April (evening sky), in the southern hemisphere at higher latitudes from around July (morning sky) to May (evening sky).

In the cycle of precession of the earth's axis, Orion currently appears at its almost northernmost position, will reach its southernmost in 13,000 years and then cannot be fully seen from Central Europe.

Orion is a mythical skyhunter, with the stars Betelgeuse (α Orionis, part of the winter triangle ) and Bellatrix (γ) forming the shoulder, the stars Rigel (β Orionis, corner of the winter hexagon ) and Saiph (κ) forming the feet. The belt stars Alnitak , Alnilam and Mintaka (ζ, ε and δ Orionis) in a strongly overstretched angle are also called three kings , Jacob's staff or Jacob's ladder and are part of the open star cluster Cr 70 .

The main stars - apart from the red giant Betelgeuse - are of a similar age and size , which suggests that they originated together.

In the lower half in the middle of Orion's “sword hanger”, the emission nebula  with the brightest surface area can be seen with the naked eye as Orion Nebula M 42 . The pronounced star formation area surrounds the trapezoidal stars θ 1  Orionis and θ 2  Orionis and represents the shining tip of an extensive cloud complex of interstellar matter that pervades the entire constellation. To the north over M42 is the part nebula M43 , also known as the Little Orion Nebula or de Mairan's Nebula .

A chain of stars is called a "sword hanger" and is composed of M42, θ and ι Orionis from north to south. To the north is the open star cluster NGC  1981.

The approximately 8 ° long arc of the weaker stars π 1 , π 2 , π 3 , π 4 , π 5 and π 6 Orionis is interpreted in various old representations as a club, a bow and Albrecht Dürer's cloak.

The star Meissa (λ Orionis), which marks Orion's head, is in the open star cluster Cr 69 .

About half a degree south of the left belt star Alnitak is the famous Horsehead Nebula B  33, a dark cloud clearly visible in front of the emission nebula IC  434.

In Orion there is also the emission nebula Barnard's Loop , which stretches around the belt stars in a wide arc of about 12 ° in diameter from the north and extends to near Rigel in the south .

history

20180211 Orion, main stars (02259) .jpg
The main stars in the southern winter starry sky
Orion constellation.jpg
... and labeled


Orion with glowing red clouds of ionized hydrogen (H-alpha).
The great arc is called Barnard's Loop . (Long-term recording)
Orion in the visible and in the infrared spectral range
Orion: The spectral classes can be recognized by the different colors of the star trails. (Photo: exposure time approx. 600 s, on Agfacolor L UT 18, Karlsruhe)

Because of its conspicuousness, various meanings were ascribed to the constellation by peoples of ancient times:

The Sumerians saw it as a sheep . With them, Betelgeuse, which is sometimes translated from Arabic as "armpit", was the "armpit of the sheep".

The Egyptians saw it as a reflection of their god Osiris .

The ancient Greeks identified the constellation with the great hunter Orion . Orion is mentioned in Horace 's Odes , Homer's Odyssey and Iliad, and in Virgil's Aeneid .
The name of the constellation may be older than Greek mythology itself. It is sometimes assumed that the name is derived from the Akkadian Uru-anna , "light of the sky", and was later adopted by the Greeks . It is also believed that the Greeks adopted the heroic figure from the Sumerian- Babylonian epic about Gilgamesh , the mythical king of Uruk .

The Teutons recognized a plow in the constellation .

The Vikings often found the interpretation of the god Thor , who wades through a river and pulls the god Loki over, hanging on his belt.

In ancient China , the constellation was one of the 28 “residences” ( Chinese  宿 , Pinyin xìu ) in the Chinese star constellations . It is referred to as Shen , which means "three" and probably comes from the three belt stars.

For the islanders of the South Seas , the constellation represented a war boat or a butterfly.

In the Coelum Stellatum Christianum by Julius Schiller it is called Saint Joseph.

mythology

There are different versions of Orion's life and work in Greek mythology :

He is said to have been the son of the sea god Poseidon , who freed the island of Chios from wild animals. However, when he raped Merope , the daughter of King Oenopion , he was blinded by her father as a punishment . Orion walked blindly to the east to be healed by the rays of the morning sun. Eos , the goddess of the dawn, fell in love with him instantly. The chaste goddess of the hunt, Artemis, grudged the young man and shot him with an arrow. Orion and the Pleiades were immortalized in the sky, the latter as "seven stars".

According to another version, Artemis wanted to renounce her vow of chastity out of love for Orion. Her twin brother Apollon , who wanted to prevent this, used a trick. He persuaded Artemis to practice archery and aim for the ocean waves while Orion swam there. Orion was fatally struck by an arrow. The grieving Artemis took her lover to heaven.

In another narration, Orion boasted that he was the greatest hunter in the world, which Zeus ' wife Hera resented. She sent out a scorpion that stabbed Orion fatally. God Zeus then transfers both of them to heaven. When the constellation of Scorpio rises in the east, Orion must leave the sky in the west. As a result, the two opponents are never together in the sky.

Celestial objects

Stars

B. F. Names or
other designations
Apparent
size
(mag)
Del.
( Ly )
Spectral class
101α 58 Betelgeuse , Betelgeuse 0.0 to 1.3 0640 M1-2 Ia-Iab
102β 19th Rigel 0.03 to 0.3 0773 B8 Iab + B9 V + B9 V
103γ 24 Bellatrix 1.64 0243 B2 III
105ε 46 Alnilam 1.69 1342 B0 Iab
106ζ 50 Alnitak 1.74 0818 O9.7 Ibe + O + B0 III
110κ 53 Saiph 2.07 0722 B0.5 Iavar
104δ 34 Mintaka 2.20 to 2.35 0916 O9.5 II + B2 V
109ι 44 Nair Al Saif , Hatysa 2.75 1326 O9 III
116π 3 01 Tabit 3.19 0026th F6 V
107η 28 Eta Orionis 3.35 0901 B1 V + B2
111λ 39 Meissa 3.39 1056 O8 III + B0.5 V
119τ 20th 3.59 0555 B5 III
116π 4 03 Pi 4 Orionis 3.68 ≈1000 B2 III SB
116π 5 08th 3.71 1342 B2 III SB
118σ 48 Sigma Orionis 3.77 1149 O9.5 V
115ο 2 09 4.06 0169 K2 III
121φ 2 40 Khad Posterior 4.09 0116 G8 III-IV
112μ 61 4.12 0152 A2 Vm
200ee 29 4.13 0174 G8 III
200aA. 32 4.20 0289 B5 V
116π 2 02 4.35 0194 A1 Vn
121φ 1 37 Khad Prior 4.39 0985 B0 IV
122χ 1 54 Chi1 Orionis 4.39 0028 G0 V
113ν 67 4.42 0535 B3 IV
114ξ 70 4.45 0635 B3 IV
117ρ 1 17th 4.46 0344 K3 III
116π 6 10 4.47 0954 K2 II
124ω 47 4.50 1623 B3 IIIe
400 HR 2113 4.53 3978 K2 III
200cc 42 4.58 0786 B2 III
123ψ 2 30th 4.59 1418 B2 IV
120υ 36 Thabit 4.62 ≈3000 B0 V
122χ 2 62 4.64 B2 Ia
116π 1 07th 4.64 0121 A0 V
400 11 4.65 0400 A0V p Si
400 31 4.71 0456 K5 III
115ο 1 04th 4.71 0542 M3
400 22nd 4.72 1289 B2 IV-V
400 56 4.76 1113 K2 IIvar
400 49 4.77 0154 A4 V
400 HR 1887 4.78 1864 B0.5 V
400 15th 15 Orionis 4.81 0319 F2 IV
123ψ 1 4.89 1110 B1 V: pe
400 51 4.90 0302 K1 III
400 4.91 0507 M1 III
400 HR 1952 4.95 2091 B2 IV-V
400 69 4.95 0775 B5 Vn
400 23 4.99 0962 B1 V
400 74 5.04 0064 F5 IV-V
400 27 5.07 0172 K0 III
108θ 2 5.08 O9.5 PU
400 64 5.14 1070 B8 V
400 HR 1684 5.18 0321 K5 III
400 06th 5.18 0241 A3 V
400 71 5.20 0069 F6 V
400 60 5.21 0367 A1 Vs
400 45 5.24 0371 F0 III
400 52 5.26 0480 A5 V
400 38 5.32 0345 A2 V
400 05 5.33 0638 M1 III
400 HR 1571 5.33 0441 K1 III
400 14th 5.33 0194 At the
400 72 5.34 0480 B7 V
400 21st 5.34 0198 F5 IIvar
400 HR 1861 5.34 2569 B1 IV
400 HR 1519 5.35 0267 At the
400 HR 1868 5.36 1853 B1 V
400 55 5.36 1681 B2 IV-V
400 75 5.39 0254 A2 V
400 HR 1507 5.39 0157 F0 V
400 U 5.40 2146 M6 e - M9.5 e
400 16 5.43 0176 A2 w
400 73 5.44 1400 B9 II-III
400 33 5.46 1568 B1.5 V
400 HR 1709 5.50 0599 K4 III
400 HD 37605 8.7 0143 K0

Bellatrix (γ Orionis), the third brightest star in Orion, is a reddish shining star 243 light years away. It has 4,000 times the luminosity of our sun . The name Bellatrix is Latin and means "warrior".

ε Orionis, the middle of the belt stars, is a bluish-white supergiant 1,340 light-years away. The name Alnilam is of old Arabic origin and means “string of pearls”.

Multiple stars

The three belt stars of Orion . Flame Nebula and Horsehead Nebula (bottom left) can only be clearly observed photographically
system Sizes (mag) distance
β 0.3 / 6.8 / 6.8 09.8 "
θ 1 diverse diverse
ι 2.8 / 6.9 11.3 "
λ 3.6 / 5.5 04.4 "
σ five times (4.0 to 9.5) see σ Ori
o², ο¹ 4.1 / 4.6 opt. Double star

Rigel (β Orionis) is the seventh brightest star in the night sky despite its distance of 770 light years. It is a binary star system . The main star is a blue giant with 17 times the mass, 60 times the diameter and 40,000 times the luminosity of our sun . This makes it one of the most luminous stars in our Milky Way . In the telescope a companion star of 6th magnitude is visible. The observation is not very easy, because the 0.1 m bright main star outshines the companion. The main star pulsates slightly, changing its brightness by 0.03 to 0.3 meters over a period of about 25 days . The old Arabic name Rigel is derived from "the left foot".

Theta 1 Orionis is a part of a star cluster, also known as a trapezoid (asterism). The Washington Visual Double Star Catalog has 42 entries, 18 of which are double stars.

ζ Orionis, the left belt star, is a triple star 817 light years away. A companion star of the 4th magnitude can already be observed with a small telescope.
The Arabic name Alnitak means "belt".

δ Orionis, the right belt star, is also a triple star. The system is 916 light years away. A companion star with a brightness of 6.9 m becomes visible in the telescope . The 2.2 m bright main star still has a close companion, which can only be detected spectroscopically .

σ Orionis is even a fivefold star . Around the spectroscopic double star (small companion 0.3 "apart), C, D and E are currently 11 to 43" apart.

Omikron Orionis is an optical (only apparent) double star. Around 1895 it was assumed from anomalies in the line spectrum of o 2 that it could be multiple. However, recent measurements have not confirmed this.

Variable stars

star Apparent Size (mag) period Type
α 0.0 to 0.9 420 days / 6 years semi-regular (SR c)
β 0.03 to 0.3 22 to 25 days slightly irregular
δ 2.20 to 2.35 Coverage variable
U 4.8 to 12.6 372 days Mira star
W. 5.9 to 7.7 12 days semi-regular

Betelgeuse (α Orionis) is a red supergiant about 640 light years away. It has about 15 times the mass and 630 times the diameter of the sun. If the star were in the center of the solar system , it would protrude beyond the orbit of Mars . Betelgeuse is a single star. However, there are indications that it might have incorporated a companion star about one solar mass when it expanded into a red giant about 100,000 years ago. It is a variable star , the brightness of which changes significantly over a period of about 6 years and is usually lower than that of Rigel (β Ori). At the end of 2019 Betelgeuse even passed through a century minimum weaker than 1.7 mag , possibly triggered by extensive star spots . The star has reached the end of its evolution and is expected to explode as a Type II supernova within the next 100,000 years .

The name comes from the Arabic يد الجوزاء, DMG yad al-ǧauzāʾ ("hand of the [constellation] twin", "hand of the giantess"). It already appears in the book of the constellations of the fixed stars by the Arab astronomer Abd ar-Rahman as-Sufi († 986).

The current German name form arose because the Arabic first letter Ya (يـwith two dots) incorrectly as Ba (بـwith a dot) and thus transcribed into Latin . During the entire Renaissance period the star was called Bait al-Jschauza , with the meaning assumed in the Arabic original as "armpit of the giantess", although the correct translation of "armpit"ابط, DMG Ibṭ would have been. This is where the name Betelgeuse came from .

Messier and NGC objects

Messier (M) NGC other Size ´ (mag) Type Surname
1662 6.4 Open star cluster
42 1976 4.0 Emission nebula Orion Nebula
43 1982 9.0 Emission nebula small Orion Nebula
78 2068 8.0 Reflection fog
1977 7.0 Reflection fog
1980 2.5 Open star cluster and nebula
1981 4.2 Open star cluster
1999 Reflection fog Keyhole Nebula
2024 diffuse fog Flaming tree
2071 8.0 diffuse fog
IC 434 Emission nebula with Horsehead Nebula
2169 5.9 Open star cluster
2175 Open star cluster with gas nebula
2186 8.7 Open star cluster
2194 8.5 Open star cluster
Amateur astronomical image of the Orion Nebula

M 42 and M 43, the Orion Nebula 1400 light years away , is one of the most beautiful observation objects in the night sky. Even in binoculars it can be seen as a foggy structure. The four brightest trapezoidal stars in the nebula can be observed in a small telescope. Six stars are visible in a telescope with an aperture of 10 cm or more. The stars stimulate the surrounding gas clouds to glow, which reveal fascinating details in the telescope.

Another well-known object is a cloud of dust that appears in front of the emission nebula IC 434 and is called the Horsehead Nebula because of its shape . Although the cloud is large, observing it is difficult, even with large telescopes, due to the low surface brightness. Long exposure photographs show details.

See also

Web links

Commons : Orion  - collection of images, videos and audio files

Individual evidence

  1. ^ Elijah Hinsdale Burritt, The Geography of the Heavens , Boston, 1833 (p. 53)
  2. Greek and Roman gods and legendary figures
  3. Orion and the Pleiades
  4. Constellation Myths - Orion
  5. Constellation description - Orion constellation
  6. ^ VizieR database
  7. Ladislaus Weinek : Atlas der Himmelskunde , Verlag Hartleben, Vienna-Pest-Leipzig 1898, p. 146.
  8. Is Betelgeuse a cosmic cannibal?
  9. Star spots darkened Betelgeuse
  10. ^ A b Paul Kunitzsch, Tim Smart: A Dictionary of Modern Star Names . Sky Publishing, Cambridge MA 2006, ISBN 978-1-931559-44-7 , pp. 45 .