GIOTTO-Halley encounter - When was the large nutation generated?

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

6

Giotto Mission, Halley'S Comet, Meteoritic Damage, Radio Communication, Spacecraft Communication, Angular Momentum, Electric Discharges, Nutation, Radio Astronomy, Telemetry

Scientific paper

It is generally believed that a very large dust particle with mass greater than 100 mg hit the GIOTTO spacecraft 7.6 sec before encounter, induced the switchover from the primary X-band amplifier (TWT) the redundant unit, generated the observable post-encounter nutation of about 1 deg and was responsible for the 22 sec telemetry loss during the phase of closest approach to Comet Halley. Using the data of the GIOTTO Radio-Science Experiment (GRE), it is shown that the signal loss was caused by an off-pointing of the antenna dish. The drop in signal level, however, is not consistent with the spacecraft having a nutation of 1 deg at this time. It is concluded that the off-pointing of the antenna dish is most likely due to an error in the High Gain Antenna (HGA) Design Control System resulting from an electrical discharge at t(0) - 8 sec and that the large nutation was generated during the telemetry blackout by the impacts of several large dust particles in the interval from 2 sec before to 18 sec after encounter.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

GIOTTO-Halley encounter - When was the large nutation generated? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with GIOTTO-Halley encounter - When was the large nutation generated?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GIOTTO-Halley encounter - When was the large nutation generated? will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1787350

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.