Hertzsprung gap

The Hertzsprung Gap is a feature of the Hertzsprung–Russell diagram for a star cluster. It is named after Ejnar Hertzsprung, who first noticed the absence of stars in the region of the Hertzsprung–Russell diagram[1] between A5 and G0 spectral type and between +1 and −3 absolute magnitudes (i.e. between the top of the main sequence and the red giants for stars above roughly 1.5 solar mass. When a star during its evolution crosses the Hertzsprung gap, it means that it has finished core hydrogen burning, but has yet to start hydrogen shell burning.

Hertzsprung–Russell diagram with the Hertzsprung Gap visible as an area containing few stars between the main sequence and red giant branch

Stars do exist in the Hertzsprung gap region, but because they move through this section of the Hertzsprung–Russell diagram very quickly in comparison to the lifetime of the star (thousands of years, compared to tens of billions of years for the lifetime of the star[2]), that portion of the diagram is less densely populated. Full Hertzsprung–Russell diagrams of the 11,000 Hipparcos mission targets show a handful of stars in that region.[3]


References
  1. Hoyle, F (May 7, 1959). "On The Main-Sequence Band and the Hertzsprung Gap". Monthly Notices of the Royal Astronomical Society. 120: 22. Bibcode:1960MNRAS.120...22H. doi:10.1093/mnras/120.1.22.
  2. Binney, J. and Merrifield, M., "Galactic Astronomy," Table 5.2, Figure 5.2, pp. 266–271.
  3. Binney, J. and Merrifield, M., "Galactic Astronomy," Figure 3.5, pp. 102–103, p. 265.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.