Threats to Earth

Threats to Earth

The aim of this lecture is to present on threats to Earth. Here briefly describe about the properties of asteroids and how asteroids have affected Earth…
Nonlinear Schrödinger Equation

Nonlinear Schrödinger Equation

Nonlinear Schrödinger Equation can be applied to hydrodynamics, nonlinear optics, nonlinear acoustics, quantum condensates, heat pulses in solids and various other nonlinear instability phenomena. It…
Jupiter: King of Planets

Jupiter: King of Planets

Principle objective of this lecture is to present on Jupiter: King of Planets. Jupiter is the largest planet in the solar system. Fittingly, it was named after…
Distance of our Solar Neighborhood

Distance of our Solar Neighborhood

Major objective of this lecture is to present on distance of our Solar Neighborhood. Knowing the distances to our stellar neighbors can help us learn…
Celestial Objects to Scale

Celestial Objects to Scale

The aim of this lecture this to present on Celestial Objects to Scale. Here briefly present on astronomical magnitude scale. The ANU SkyMapper telescope is surveying the Southern…
What are Mass and Weight?

What are Mass and Weight?

Prime objective of this lecture is to present on Mass and Weight. Mass is the amount of matter in an object and is measured in kilograms. It is…
Exploring our Solar System

Exploring our Solar System

General objective of this lecture is to present on Exploring our Solar System. Our solar neighborhood is an exciting place. The Solar System is full of planets,…
Deep Impact

Deep Impact

Principal Investigator, Dr. Michael A’Hearn and his science team want to find clues to the formation of the solar system and more about the structure…
Fluid Dynamics

Fluid Dynamics

Fluid Dynamics provides methods for studying the evolution of stars, ocean currents, weather patterns, plate tectonics and even blood circulation. It is the branch of…
Cosmic Rays and Solar Flares

Cosmic Rays and Solar Flares

Basic purpose of this lecture is to present on Cosmic Rays and Solar Flares. Cosmic rays are fast-moving ionising particles from the Sun. The Earth’s magnetic field prevents…
Navier–Stokes Equations

Navier–Stokes Equations

Navier-Stokes Equations are time-dependent and consist of a continuity equation for conservation of mass, three conservation of momentum equations and a conservation of energy equation.…
Lecture on Galaxies

Lecture on Galaxies

Galaxies are large assembly of stars and nebulae. Most galaxies are billions of years old. The youngest known galaxy is 1 Zwicky 18. At an estimated…
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