Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-26T05:10:46.745Z Has data issue: false hasContentIssue false
  • English
  • Français

1.1.18 Presentation of Zodiacal Light Instrument Aboard the D2B Astronomical Satellite

Published online by Cambridge University Press:  12 April 2016

M. Maucherat  and
P. Cruvellier
M. Maucherat
Affiliation:
Laboratoire d’Astronomie Spatiale, Marseille
P. Cruvellier
Affiliation:
Laboratoire d’Astronomie Spatiale, Marseille

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The french astronomical satellite D2B is to be launched on September 1975. During the dial of the orbit, one axis of the satellite points to the Sun, with an accuracy of ± 30 arcmin; during the night of the orbit, the satellite keeps this stabilization by gyroscopic effect. The perpendicular axes -one of them is the optical axis of the Z.L. (Zodiacal Light) instrument- roll around the Earth-Sun direction, once every 4 minutes. Because of the Earth’s motion around the Sun, the celestrial sphere will be scanned along ecliptic meridians, every orbits; the complete exploration of the sky will be achieved after six months. The Z.L. instrument is a photometer analyzing galactic and zodiacal fluxes, in the range λλ 3100-750, in five spectral intervals 200-500 wide, with a field of 2.8°□. For a single scan, the limit of detection by the instrument will be the 6th visual magnitude for early-type stars (0-B).

Type
1 Zodiacal Light
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 74 - 77
Copyright
Copyright © Springer-Verlag 1976

References

Davidsen, A., Bowyer, S., Lampton, M. 1974, Nature 247, 513.Google Scholar
Dumont, R., Sanchez-Martinez, F. 1966, Ann. Astrophys. 29, 113.Google Scholar
Dumont, R., Sanchez-Martinez, F. 1973, Astron. Astrophys. 22, 321.Google Scholar
Frey, A., Hofmann, W., Lemke, D., Thum, C. 1974, Astron. Astrophys. 36, 447.Google Scholar
Habing, H.J. 1968, Bull. Astr. Inst. Netherlands 19, 421.Google Scholar
Henry, R.C. 1973, Astrophys. J. 179, 97.Google Scholar
Lillie, C.F. 1972, Scientific Results from OAO-2, 95 (NASA, 1972).Google Scholar