Perseus Arm

The Perseus Arm is one of two major spiral arms of the Milky Way galaxy. The second major arm is called the Scutum–Centaurus Arm. The Perseus Arm begins from the distal end of the long Milky Way central bar.[1] Previously thought to be 13,000 light-years away from Earth, research published in 2005 has suggested that it is less than half that distance, estimated at 6,400 light years, from the Solar System.[2]

Overview

The Milky Way is a barred spiral galaxy with two major arms and a number of minor arms or spurs.[1] The Perseus Spiral Arm, with a radius of approximately 10.7 kiloparsecs, is located between the minor Cygnus and Carina–Sagittarius Arms.[1] It is named after the Perseus constellation in the direction of which it is seen from Earth.

Scientists in two large radio astronomy projects – the Japanese VLBI Exploration of Radio Astrometry (VERA), which launched its efforts in 2001,[3] and the Bar and Spiral Structure Legacy (BeSSeL) Survey, which launched its efforts in 2010,[4] – made great efforts over about 20 years to measure the trigonometric parallaxes toward about 200 water vapor (H
2O) and methanol (CH
3OH) masers in massive star-forming regions in the Milky Way. They have employed these parallax measurements to delineate the forms of spiral arms from the Galactic longitude 2 to 240 degrees and extended the spiral arm traces into the portion of the Milky Way seen from the Southern Hemisphere using tangencies along some arms based on carbon monoxide emission. The image clearly presents the Milky Way as a barred spiral galaxy with fairly symmetric four major arms and some extra arm segments and spurs.[5][6]

The Perseus Arm is one of the four major arms. The arm is the length of more than 60,000 lr and the width of about 1,000 lr and the spiral extension in the pitch angle near 9 degree.[5]

There is speculation that the local spur known as the Orion–Cygnus Arm, which includes the Solar System and Earth and is located inside of the Perseus Arm,[1] or is a branch of it, but this is unconfirmed.

The Perseus Arm contains the Double Cluster and a number of Messier objects:

See also

References

  1. ^ a b c d Churchwell, Ed; Babler, Brian L.; Meade, Marlin A. (2009). "The Spitzer/GLIMPSE Surveys: A New View of the Milky Way" (PDF). Publications of the Astronomical Society of the Pacific. 121 (877): 213–230. Bibcode:2009PASP..121..213C. doi:10.1086/597811.
  2. ^ McKee, Maggie (8 December 2005). "Spiral arm of Milky Way looms closer than thought". New Scientist. Reed Business Information Ltd. Retrieved 31 October 2013.
  3. ^ "VLBI" (Press release). National Astronomical Observatory of Japan. 2001. Retrieved 2026-02-18. ...to make a map of the entire Milky Way Galaxy and to measure its movement
  4. ^ "BeSSeL Survey (Bar and Spiral Structure Legacy Survey)" (Press release). National Radio Astronomy Observatory. 2010. Retrieved 2026-02-18. The goal of BeSSeL is to measure accurate distances and proper motions of up to 400 high mass star forming regions in the Milky Way between 2010 and 2015.
  5. ^ a b Reid, M. J.; et al. (2009). "Trigonometric parallaxes of massive star-forming regions. VI. Galactic structure, fundamental parameters, and noncircular motions". The Astrophysical Journal. 700 (1): 137–148. arXiv:0902.3913. Bibcode:2009ApJ...700..137R. doi:10.1088/0004-637X/700/1/137. S2CID 11347166.
  6. ^ Hirota, Tomoya; et al. (2020). "The First VERA Astrometry Catalog". Publications of the Astronomical Society of Japan. 72 (4). arXiv:2002.03089. doi:10.1093/pasj/psaa018.
This article is issued from Wikipedia. The text is available under Creative Commons Attribution-Share Alike 4.0 unless otherwise noted. Additional terms may apply for the media files.