Abstract
Recent claims of small icy comets disintegrating in the high atmosphere point to a component of comets in the form of loose aggregates of dust. This could be understood in terms of Lyttleton;'s theory of comet formation by accretion of interstellar grains.
Similar content being viewed by others
References
Frank, L.A.: 1997, internet release http://smallcomets.physics.uiowa.edu/www/may28-1.html.
Frank, L.A. and Sigwarth, J.B.: 1997a, Geophys. Res. Lett., 24, 2423.
Frank, L.A. and Sigwarth, J.B.: 1997b, Geophys. Res. Lett., 24, 2431.
Frank, L.A. and Sigwarth, J.B.: 1997c, Geophys. Res. Lett., 24, 2427.
Frank, L.A. and Sigwarth, J.B.: 1997d, Geophys. Res. Lett., 24, 2435.
Hoyle, F.: 1949, Some Recent Researches in Solar Physics, Cambridge University Press.
Lyttleton, R.A.: 1952, Comets and their Origin, Cambridge University Press.
Rights and permissions
About this article
Cite this article
Hoyle, F., Wickramasinghe, C. Small Comets in the High Atmosphere. Astrophysics and Space Science 253, 13–17 (1997). https://doi.org/10.1023/A:1000412523886
Issue Date:
DOI: https://doi.org/10.1023/A:1000412523886