Inaugurator of geography/coining of term
Eratosthenes
Shape of earth
Geoid- spherical but flattened at poles
Geographical Information system (GIS)
Collects and manipulates data to create maps
Global Navigation Satellite System (GNSS)
To find out the exact location of something on the earth. Also called GPS (USA), GLONASS (Russia), IRNSS (India) etc.
Theories of the origin of planets/ earth
Nebular hypothesis by Laplace and Immanuel Kant- from cloud of rotating material
Chamberlain and Moulton considered that a wandering star approached the sun. As a result, a cigar-shaped extension of material was separated from the solar surface. As the passing star moved away, the material separated from the solar surface continued to revolve around the sun and it slowly condensed into planets
Accretion theory- Schmidt and Weizascar- nebula of hydrogen helium spun and collapsed on itself due to gravity, forming disc shaped cloud and clumps and bunching- heavier stuff stuck together (rocky planets), lighter flew away (gas giants).
Origin of the universe theory
Big Bang theory/expanding universe hypothesis by Lemaitre and Hubble- 13.75 billion years ago rapid expansion in a millisecond from a single atom of small volume, infinite temperature and infinite density, it exploded, some energy converted to matter, Within 300,000 years from the Big Bang, temperature dropped to 4,500 K (Kelvin) and gave rise to atomic matter. The universe became transparent.
Hoyle’s concept of steady state. It considered the universe to be roughly always the same.
Formation of stars
Nebula (cloud of matter) develops localised clumps of gas. These clumps continue to grow into even denser gaseous bodies, giving rise to formation of stars.
Earth age
4.6 billion years
Evolution of lithosphere of the earth
Separation of material into different layers depending upon density. Heavy sank to centre, lighter floated upwards. With time, cooling, solidification and condensation into crust. Moon collision further shook things up before settling again. Differentiation.
Evolution of Atmosphere of the earth
The first stage is marked by the loss of the primordial atmosphere of hydrogen and helium due to solar winds. In the second stage, the interior of the earth released gases (nitrogen, carbon dioxide, methane, ammonia and very little free oxygen) The process through which the gases were outpoured from the interior is called degassing and water vapour condensed contributed to the evolution of the atmosphere. Finally, the composition of the atmosphere was modified by the living world through the process of photosynthesis.
Evolution of Hydrosphere of the earth
Degassing (through volcanic eruptions) contributed water vapour and gases to the atmosphere. As the earth cooled, the water vapour released started getting condensed. The carbon dioxide in the atmosphere got dissolved in rainwater and the temperature further decreased causing more condensation and more rains. The rainwater falling onto the surface got collected in the depressions to give rise to oceans. The earth’s oceans were formed within 500 million years from the formation of the earth. Sometime around 3.8 billion years ago, life began to evolve. However, around 2.5 billion years before the present, the process of photosynthesis evolved. Oceans began to have the contribution of oxygen through the process of photosynthesis. Eventually, oceans were saturated with oxygen, and 2 billion years ago, oxygen began to flood the atmosphere.
Inner and outer planets
mercury, venus, earth and mars are called as the inner planets as they lie between the sun and the belt of asteroids the other four planets are called the outer planets.
Jovian planets
The outer four are called Jovian or Gas Giant planets. Jovian means jupiter -like.
Difference between terrestrial and jovian planets
(i) The terrestrial planets were formed in the close vicinity of the parent star where it was too warm for gases to condense to solid particles. Jovian planets were formed at quite a distant location.
(ii) The solar wind was most intense nearer the sun; so, it blew off lots of gas and dust from the terrestrial planets. The solar winds were not all that intense to cause similar removal of gases from the Jovian planets.
(iii) The terrestrial planets are smaller and their lower gravity could not hold the escaping gases.
Moon formation
Sir George Darwin suggested that initially, the earth and the moon formed a single rapidly rotating dumbbell shaped body, and it broke off. Now believed that outcome of ‘giant impact’ or “the big splat”. A body of the size of one to three times that of mars collided into the earth, blasted a large part into space which eventually formed into the present moon about 4.44 billion years ago.
Evolution of life on earth
Modern scientists refer to the origin of life as a kind of chemical reaction, which first generated complex organic molecules and assembled them. This assemblage was such that they could duplicate themselves converting inanimate matter into living substance sometime 3,800 million years ago.
Formation of planets
Nebula becomes star by bunching and clumping. The gas cloud starts getting condensed and the matter around the core develops into small- rounded objects by the process of cohesion and collision develop into planetesimals. Large number of small planetesimals accrete to form a fewer large bodies in the form of planets.
Phases of the moon
Full Moon- Poornima- once a month, entire visible
New Moon- Amavasya- completely disappeared
Each occur a fortnight apart
Celestial bodies
Objects shining in the night sky
Stars
Made up of gasses, emit their own heat and light. Sun, and nearest to it is Proxima Centauri
Constellations
Patterns formed by stars
Pole Star
Aka north star, fixed position and indicates north
Planets
Celestial bodies that do not emit own heat and light
Planets in solar system number and name
8- Mercury venus earth mars jupiter saturn uranus neptune