Trapezium Cluster

Source: Wikipedia, the free encyclopedia.
For other stars with this Bayer designation, see θ Orionis.
Trapezium
Distance
1,344±20 ly (412 pc[1])
Apparent magnitude (V)4.0
Apparent dimensions (V)47 (seconds of arc)
Physical characteristics
Mass? M☉
Radius10 ly
Estimated age300,000 years
Associations
ConstellationOrion
See also: Open cluster, List of open clusters
Three of the main stars of the Trapezium, with the triple star in the top right, as sketched by Galileo. The letters do not correspond to the current designations.

The Trapezium or Orion Trapezium Cluster, also known by its Bayer designation of Theta1 Orionis (θ1 Orionis), is a tight open cluster of stars in the heart of the Orion Nebula, in the constellation of Orion. It was discovered by Galileo Galilei. On 4 February 1617 he sketched three of the stars (A, C and D), but missed the surrounding nebulosity.[2][3][4] A fourth component (B) was identified by several observers in 1673, and several more components were discovered later like E, for a total of eight by 1888. Subsequently, several of the stars were determined to be binaries. Telescopes of amateur astronomers from about 5-inch (130 mm) aperture can resolve six stars under good seeing conditions.[5]

The Trapezium is a relatively young cluster that has formed directly out of the parent nebula. The five brightest stars are on the order of 15 to 30 solar masses in size. They are within a diameter of 1.5 light-years of each other and are responsible for much of the illumination of the surrounding nebula. The Trapezium may be a sub-component of the larger Orion Nebula Cluster, a grouping of about 2,000 stars within a diameter of 20 light-years.

Identification

The Trapezium is most readily identifiable by the

eclipsing binaries
.

runaway stars
have been identified.

Possible black hole

A 2012 paper suggests an intermediate-mass black hole with a mass more than 100 times that of the Sun may be present within the Trapezium, something that could explain the large velocity dispersion of the stars of the cluster.[6]

  • One of the components of the cluster (Theta1 Orionis F, lower left) is a double star.[7]
    One of the components of the cluster (Theta1 Orionis F, lower left) is a double star.[7]
  • The Chandra X-ray Observatory view of the Orion Nebula
    The Chandra X-ray Observatory view of the Orion Nebula
  • Trapezium star identification
    Trapezium star identification
  • Hubble detail of a region west of the Trapezium, showing arcs and bubbles formed when stellar winds collide with existing interstellar material
    Hubble detail of a region west of the Trapezium, showing arcs and bubbles formed when stellar winds collide with existing interstellar material
  • A wider shot of the core details showing the trapezium in context of the surrounding nebulae
    A wider shot of the core details showing the trapezium in context of the surrounding nebulae
  • Core detail of the nebula with all the stars identified
    Core detail of the nebula with all the stars identified

List of stars

Main article: Theta Orionis
Star Stellar components
A

A1, A2, A3

B

B1, B2, B3, B4, B5

C

C1, C2

D

/

E

E1, E2

F

F1, F2

G

/

H

/

References

  1. ^ Reid, M. J.; et al. (2009). "Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions".
    S2CID 11347166
    .
  2. ^ Galileo Galilei: Siderius Nuncius, Venice, 1610. English Translation published at Bard College, Hudson, New York, October 9, 2003 English Translation [1] Archived 2004-07-06 at the Wayback Machine Original Latin version [2]
  3. ^ Tom Pope and Jim Mosher: Galilean telescope homepage" March 17, 2006 "The Trapezium Through the Galilean Telescope". Archived from the original on 2008-01-30. Retrieved 2008-01-30., "Some have expressed puzzlement that in his text Galileo does not mention the nebulosity (known in modern nomenclature as M42) enveloping these stars. ... Galileo believed, as he explains in Sidereus Nuncius, that what looks nebulous to the eye is resolved into stars by his telescope; what looks nebulous through his telescope could presumably also be resolved into stars by a still larger and more powerful telescope. Hence, a diffuse glow would be, more than anything, an indication of the limitations of his telescope and not particularly worthy of special note."
  4. ^ Tom Pope and Jim Mosher: Page on Galileo's February 4, 1617 notebook drawing of the Trapezium region, May 2, 2006 "Perhaps significantly, Galileo makes no mention of having noticed the now well-known gas cloud, M42, surrounding the Trapezium stars."[3] Archived 2011-08-11 at the Wayback Machine
  5. ^ "Trapezium Cluster". 15 May 2015. Retrieved 2018-03-06.
  6. S2CID 118549761
    .
  7. ^ "First Light For Future Black Hole Probe". Retrieved 15 January 2016.

Further reading

External links

Wikimedia Commons has media related to Trapezium (astronomy).
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