The historical investigation of cometary brightness

Details The historical investigation of cometary brightness The historical investigation of cometary brightness

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jahh....1..123h&link_type=abstract

Journal of Astronomical History and Heritage (ISSN 1440-2807), Vol. 1, No. 2, p. 123-133 (1998).

Astronomy and Astrophysics

Astronomy

2

Comet, Brightness, Nucleus, Solar System

Scientific paper

The interpretation of the way in which the brightness of a comet varied as a function of both its heliocentric and geocentric distance was essentially started by Isaac Newton in his book Philosophiae Naturalis Principia Mathematica, published in 1687. Astronomers have argued about the form of this variability ever since, and for many years it was regarded as an important clue as to the physical nature of the cometary nucleus and its decay process. This paper reviews our understanding of the causes of cometary brightness variability between about 1680 and the 1950s.

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