Solar apex

Summary

Solar apex
Solar apex.png
(RA) 18h 28m 0s (dec) 30°N
Solar antapex
Solar antapex.png
(RA) 6h 28m 0s (dec) 30°S
The movement of stars of spectral classes B and A around the apex (left) and antapex (right) in ± 200 000 years.

The solar apex, or the apex of the Sun's way, refers to the direction that the Sun travels with respect to the local standard of rest. This is not to be confused with the Sun's apparent motion through all constellations of the zodiac, which is an illusion caused by the orbit of the Earth.

Direction

The solar apex is in the constellation of Hercules, southwest of Vega, northeast of his "outstretched arm", Omicron Herculis.[1] There are two mainstream sets of coordinates for the solar apex.

  • The radioastronomical position is RA 18h 03m 50.2s, dec +30° 00′ 16.8″ (galactic coordinates: 58.87° longitude, 17.72° latitude).

Evaluation of movement of the solar system in its neighborhood is complex; a selection of links is on the Talk page of this article.

For more than 30 years before 1986 the speed of the Sun towards the solar apex was taken to be about 20 km/s[2] but all later studies give a smaller component in the vector toward galactic longitude 90°, reducing overall speed to about 13.4 km/s.[3] This speed is not to be confused with the orbital speed of the Sun around the Galactic center, which is about 220 km/s and is included in the movement of the Local Standard of Rest. Thus the Sun moves towards the apex (a relatively local point) at about 113 our spiral arm's orbital speed. The sun's motion in the Milky Way is not confined to the galactic plane; it also shifts ("bobs") up and down with respect to the plane over millions of years.[4]

History

The nature and extent of the solar motion was first demonstrated by William Herschel in 1783, who also first determined the direction for the solar apex, as Lambda Herculis, 10° away from today's accepted position.[5][6][7]

Solar antapex

The solar antapex, the direction opposite of the solar apex, is located near the star Zeta Canis Majoris.[1]

Gallery

References

  1. ^ a b Kaler, Jim. "Furud". Retrieved 2017-04-26.
  2. ^ Kerr, Frank J.; Lynden-Bell, Donald (August 1986). "Review of Galactic Constants". Monthly Notices of the Royal Astronomical Society. Bibcode:1986MNRAS.221.1023K. doi:10.1093/mnras/221.4.1023. See also Table 3 on page 13 of Kogut, A.; et al. (1993). "Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps". Astrophysical Journal. 419: 1. arXiv:astro-ph/9312056. Bibcode:1993ApJ...419....1K. doi:10.1086/173453.
  3. ^ U, V, and W (vectors) are c. 10.0, 5.25 and 7.17 km/s respectively, Dehnen, Walter; Binney, James J. (1998). "Local Stellar Kinematics from Hipparcos Data". Monthly Notices of the Royal Astronomical Society. arXiv:astro-ph/9710077. Bibcode:1998MNRAS.298..387D. doi:10.1046/j.1365-8711.1998.01600.x.
  4. ^ Frisch, Priscilla (2000); "The Galactic Environment of the Sun", American Scientist, volume 88, number 1, page 52
  5. ^ Lankford, John (1997). History of Astronomy: An Encyclopedia. Garland Encyclopedias in the History of Science. 1. Taylor & Francis. p. 258. ISBN 0-8153-0322-X.
  6. ^ Herschel, William (1783). "On the Proper Motion of the Sun and Solar System; With an Account of Several Changes That Have Happened among the Fixed Stars since the Time of Mr. Flamstead [sic]". Philosophical Transactions of the Royal Society of London. 73: 247–83. doi:10.1098/rstl.1783.0017. JSTOR 106492.
  7. ^ Hoskin, Michael (1980), "Herschel's Determination of the Solar Apex", Journal for the History of Astronomy, 11: 153–163, Bibcode:1980JHA....11..153H, doi:10.1177/002182868001100301.