Geology - the science that pursues an understanding of the Earth, its origin and history, the processes that shaped it, and the resources that could be obtained from it
Geology - scientific study of the earth's materials, processes, and its history
Orogeny - mountain-building process
Catastrophism - proposed by Baron Georges Cuvier
Catastrophism - sudden, worldwide catastrophes are the agents of change that alter the physical features of the Earth over time and the latter remains unchanged in between these periods of upheavals
Catastrophism - widely accepted by theologians in the early 1800s due to similarity with Biblical events such as the Great Flood
James Hutton - father of geology
Uniformitarianism - early idea was proposed by James Hutton and refined by John Playfair
Uniformitarianism - "The present is the key to the past."
Uniformitarianism - the Earth is continuously modified by geologic processes that have always operated throughout time (albeit different time rates).
Uniformitarianism - accepting this theory would mean that the world has been around for a very long time as opposed to the estimated made at that time
Big Bang theory - formation of the universe
Nebular theory - formation of the solar system
Big Bang theory - proposed by Georges Lemaitre in the 1920s
Big Bang theory - contends that the Universe originated from an incomprehensively large cosmic “explosion” (origin unknown) that hurled matter in all directions at incredible speed 13.7 billion years ago
During this time (big bang), the universe was also thought to be opaque.
Supernovae explosion - the very energetic explosion of massive stars created elements heavier than iron
Three main evidence supporting the Big Bang: abundance of primordial elements: primarily hydrogen and helium (and other light elements), Hubble's Law, and cosmic microwave background radiation (CMB)
Hubble's Law - galaxies seem to be moving away from us at speeds proportional to their distance
Red shift - refers to the shift of light towards longer wavelengths, often observed in the spectra of distant celestial objects, and is a key indicator of their motion away from an observer; it is a crucial piece of evidence supporting the expansion of the universe. It is a consequence of the Doppler Effect
Red shift - how we see waves when the object that is creating the waves is moving toward us or away from us
Cosmic microwave background radiation (CMB) - remnant heat of the universe, a 2.725 Kelvin signature
Arno Penzias and Robert Wilson - accidentally discovered CMB in 1965
Cosmic microwave background radiation - translates to the very small density differences of matter in the early universe and is considered as the snapshot of the oldest (microwave) light in the universe
CMB - remnant radiation
CMB - snapshot of the oldest microwave light
Main basis in determining the age of the universe - oldest objects in the universe and measuring speed of its expansion
Population III stars and globular clusters - oldest objects in the universe that gives an age limit of 11-18 billion years
Limitations of the Big Bang theory
What was present before the universe?
Will the universe end?
How will it cease to exist?
Steady-state theory - new matter is continuously created as the Universe expands
Cosmological principle - the observable universe is basically the same in any time as well as any place
Alternative theories - Steady-statetheory and DivineIntervention or Theologicaltheory
Stages in star lifetime - (1) yellow star, (2) red giant, (3) red supergiant, (4) massive red supergiant, (5) supernova
Immanuel Kant and Pierre Simon de Laplace - proposed the nebular hypothesis in the 18th century
Nebular hypothesis - suggests that the solar system originated from a single rotating cloud if gas and dust which contracted due to gravity starting 4.6 bya
Solar nebula - single rotating cloud of gas and dust
Nebula - collection of clouds of dust (very tiny grains of minerals, ice crystals, and organic particles) and gas (mostly hydrogen and helium)
The rotating gas-dust cloud began to contract due to gravity.
Accretion disk - flattened astronomical objects made of rapidly rotating gas which slowly spirals onto a central gravitating body