Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-27T06:47:36.565Z Has data issue: false hasContentIssue false

The Occultation of BD -17° 4388 by Neptune: I. Determination of Neptune’s position

Published online by Cambridge University Press:  25 April 2016

M. J. Miller*
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University, Canberra

Extract

The possibility of the occultation by Neptune of a star of similar apparent magnitude to itself was first pointed out by the amateur astronomer Ross A. Shuart. It was clear that such an event would provide data on Neptune’s position which would be of value to the observatories which produce the planetary ephemerides. The existing ephemeris of Neptune is known to contain small errors which have been accumulating over many years.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1969

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Shuart, R. A., Sky and Tel., 34, 290 (1967).Google Scholar
2 I.A.U. Circular No. 2063 (1968).Google Scholar