This website is under construction due to shifting to our new campus, inconvenience deeply regretted

Astronomy in ancient civilizations

Greek and Indian astronomy and cosmology

Copernican revolution

Galileo's vision

Tycho Brahe's measurements

Kepler's calculations

Theory of gravitation and orbits

Euler and Lagrange’s contribution

Discoveries within the solar system

From stars to galaxy and cosmology

Special and General relativity- Astronomical consequences

Contribution of quantum physics

Stellar physics and evolution

Galactic and extra-galactic astronomy and astrophysics

Modern cosmology

Clocks, globes and sundials

Telescopes, spectroscope and imaging
Photography and Detectors

X-ray astronomy

Radio astronomy

Particle astrophysics and Cosmic rays

Gravitational astronomy

Two-planet solar system Long term evolution of planetary and asteroid orbits Atmospheric drag

Rocket propulsion and dynamics Aerodynamics of rockets Wind tunnel experiments

SGP4 Propagator and TLE Sizing the debris Time of closest approach Probability of collision Removal

Geographical coordinates

Horizon system

Equatorial system

Barycentric coordinates

Galactic coordinate system

International Celestial Reference System (ICRS)

Conversion of coordinates

Apparent and real motion of the stars

Signal parameters

Rate of Arrival: Fluxes

Chain of loss of signal and calibration

Distortion and smearing and calibration

Types of noises

Sensitivity

Accuracy and precision and resolution

Estimating uncertainty

- Duaration : 4-months