Sagittarius A

Sagittarius A

Sagittarius A
Radial velocity (Rv) 46 km/s
Mass 3.7 million M
Radius R
Luminosity L
Surface gravity (log g) cgs
Temperature K
Metallicity ?
Rotation ?
Age ? years
Other designations
AX J1745.6-2900, SAGITTARIUS A, W 24, Cul 1742-28, SGR A, [DGW65] 96, EQ 1742-28, RORF 1742-289, [SKM2002] 28.
Database references

Sagittarius A (or Sgr A) is a complex radio source at the Galactic Center of the Milky Way. It is located in the Sagittarius constellation, and is hidden from view at optical wavelengths by large clouds of cosmic dust in the spiral arms of the Milky Way.

It consists of three components, the supernova remnant Sagittarius A East, the spiral structure Sagittarius A West, and a very bright compact radio source at the center of the spiral, Sagittarius A*. These three overlap: Sagittarius A East is the largest, West appears off-center within East, and A* is at the center of West.


  • Two-Dimensional Size 1
  • Spirals of Sagittarius A 2
  • Sagittarius A East 3
  • Sagittarius A West 4
  • Sagittarius A* 5
  • References 6
  • Further reading 7
  • External links 8

Two-Dimensional Size

The Two-Dimensional size of Sagittarius A* has been determined, based on Very Long Baseline Array observations, which helps explain the context of jet disk, and accretion disk models on the radio emission spectrum. These measurements were made through the use of a wavelength of 7mm, enabling the size to be determined. The result was that Sagittarius A* was determined to be an elliptical Gaussian with a semi-major axis size of 35.4x12.6 Rs with an inclination of 95 degrees east of north. The observations for this finding were found from the detection of NIR (near infrared) flares, and X-ray flares that were spotted by NuSTAR. Both flares come from electron excitation, not an enhanced accretion rate onto the black hole, which means that not all high energy events produce variability at radio wavelengths.[1]

Spirals of Sagittarius A

A study done with the measured parallaxes and motions of 10 massive regions in the spiral arms of Sagittarius in the Milky Way where stars are formed. Data was gathered using the BeSSeL Survey with the VLBA, and the results were synthesized to discover the physical properties of these sections (called the Galactocentric azimuth, around -2 and 65 degrees). The results were that the spiral pitch angle of the arms is 7.3 +- 1.5 degrees, and the half-width of the arms of the Milky Way were found to be .2 kpc. The nearest arm from the Sun is around 1.4 +- 0.2 kpc away.[2]

Sagittarius A East

This feature is approximately 25 light-years in width and has the attributes of a supernova remnant from an explosive event that occurred between 35,000 and 100,000 BCE. However, it would take 50 to 100 times more energy than a standard supernova explosion to create a structure of this size and energy. It is conjectured that Sgr A East is the remnant of the explosion of a star that was gravitationally compressed as it made a close approach to the central black hole.

Sagittarius A West

Surface brightness and velocity field of the inner part of Sagittarius A West

Sgr A West has the appearance of a three-arm spiral, from the point of view of the Earth. For this reason, it is also known as the "Minispiral". This appearance and nickname are misleading, though: the three-dimensional structure of the Minispiral is not that of a spiral. It is made of several dust and gas clouds, which orbit and fall onto Sagittarius A* at velocities as high as 1,000 kilometers per second. The surface layer of these clouds is ionized. The source of ionisation is the population of massive stars (more than one hundred OB star have been identified so far) that also occupy the central parsec.

Sgr A West is surrounded by a massive, clumpy torus of cooler molecular gas, the Circumnuclear Disk (CND). The nature and kinematics of the Northern Arm cloud of Sgr A West suggest that it once was a clump in the CND, which fell due to some perturbation, perhaps the supernova explosion responsible for Sgr A East. The Northern Arm appears as a very bright North—South ridge of emission, but it extends far to the East and can be detected as a dim extended source.

The Western Arc (outside the field of view of the image shown in the right) is interpreted as the ionized inner surface of the CND. The Eastern Arm and the Bar seem to be two additional large clouds similar to the Northern Arm, although they do not share the same orbital plane. They have been estimated to amount for about 20 solar masses each.

On top of these large scale structures (of the order of a few light-years in size), many smaller cloudlets and holes inside the large clouds can be seen. The most prominent of these perturbations is the Minicavity which is interpreted as a bubble blown inside the Northern Arm by the stellar wind of a massive star, which is not clearly identified.

Sagittarius A*

Astronomers have observed stars spinning around the supermassive black hole in Sagittarius A*.[3]

Astronomers now have evidence there is a supermassive black hole at the center of the galaxy.[4] Sagittarius A* (abbreviated Sgr A*) is agreed to be the most plausible candidate for the location of this supermassive black hole. The Very Large Telescope and Keck Telescope detected stars orbiting Sgr A* at speeds greater than that of any other stars in the galaxy. One star, designated S2, was calculated to orbit Sgr A* at speeds of over 5,000 kilometers per second at its closest approach.[5]

A gas cloud is expected to collide with the black hole in 2014 and provide additional information.[6]


  1. ^ Bower G, Law C, Ghez A, et al. The intrinsic two-dimensional size of sagittarius A*. Astrophysical Journal [serial online]. July 20, 2014;790(1)Available from: Scopus®, Ipswich, MA. Accessed October 23, 2014.
  2. ^ Wu Y, Sato M, Zheng X, et al. Trigonometric parallaxes of star forming regions in the Sagittarius spiral arm. [serial online]. April 17, 2014;Available from: arXiv, Ipswich, MA. Accessed October 23, 2014.
  3. ^ "A monster in the Milky Way". ESA/Hubble Picture of the Week. Retrieved 8 October 2013. 
  4. ^ "Black hole confirmed in Milky Way". BBC. December 9, 2008. Retrieved 2008-12-10.
  5. ^
  6. ^ It's Snack Time in the Cosmos By RON COWEN, New York Times, Feb 17, 2014

Further reading


External links

  • Recent Results of the MPE Infrared/Submillimeter Group
  • Galactic Center Research at MPE
  • report, with link to the Schödel et al. paperNature
  • Sagittarius A East
  • Kinematic and structural analysis of the Minispiral in the Galactic Center from BEAR spectro-imagery (preprint)
  • Chandra Photo Album Sagittarius A
  • The Galactic Center (outdated)
  • NASA Image of the Day Gallery 6 January 2010 Into the Heart of Darkness - Chandra X-ray Observatory image.
  • Sagittarius A at Constellation Guide