Abstract
The satellite for earth observation (Bhaskara) launched on 7 June 1979 has two TV cameras and a passive microwave radiometer for earth resources survey and meteorological studies respectively. As it had to be a minimally modified version of the earlier spin-stabilised satelliteAryabhata, it is configured as a spin-stabilised satellite, with a spin rate of between 6 to 11 rev/min and a spin axis perpendicular to the orbital plane within 3°. The cold gas system ofAryabhata was modified to provide a low and controlled thrust for spin-up and spin-axis orientation operations. Two horizon-crossing sensors are used for automatic spin-axis control and attitude determination on ground. This paper presents a report on the system evolution, design, simulation and on-orbit performance ofBhaskara.
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Abbreviations
- A:
-
wetted area of the damper
- a:
-
semi-major axis
- c d :
-
distance of the damper plane from the spacecraft co
- C f :
-
coefficient of friction between the damper fluid and wall
- d:
-
diameter of the damper tube
- e:
-
eccentricity
- g:
-
fill angle of the damper
- I X,I y :
-
moment of inertia of the satellite aboutx, y (body fixed co-ordinates) respectively
- I z :
-
moment of inertia about spin axisi.e. z-axis
- i a :
-
inclination of the orbit
- M:
-
earth’s dipole moment (- 8.06 x 1016 WM3)
- R:
-
radius of the damper
- r:
-
radius of the earth
- t:
-
time
- Ωa :
-
orbit cross-over angle from vernal equinox
- v:
-
coning angle
- v f :
-
final coning angle after some damping timet d
- vi :
-
initial coning angle
- vres :
-
residual coning angle
- ξ:
-
angle between the geomagnetic dipole moment and geometric north
- ρ:
-
density of the fluid
- ω z :
-
spin rate of the spacecraft
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Goel, P.S., Nagabushanam, S., Murugesan, S. et al. The attitude control system of the satellite for earth observation ‘ Bhaskara ’. Proc. Indian Acad. Sci. (Engg. Sci.) 5, 1–27 (1982). https://doi.org/10.1007/BF02843100
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DOI: https://doi.org/10.1007/BF02843100