The Universe and the Solar System

Learning Outcomes:

  1. Understand different theories regarding the origin and structure of the universe.
  2. Comprehend the components of the universe, including galaxies, stars, and planetary systems.
  3. Gain insight into the structure, characteristics, and components of the Solar System.
  4. Identify the features of celestial bodies like planets, stars, asteroids, comets, and meteors.

The Universe

The universe consists of all celestial bodies including stars, planets, satellites, asteroids, meteors, comets, dust, and gases. The study of these bodies is known as astronomy, with astronomers being the scientists who specialize in this field. The universe has been a subject of fascination, leading to various theories about its origin and structure.

Theories About the Universe

The understanding of the universe has evolved, primarily through two main categories of theories:

Early Theories

  1. Geocentric Theory: Proposed by Ptolemy in AD 140, it posited that the Earth was the center of the universe.
  2. Heliocentric Theory: Introduced by Copernicus in AD 1543, suggesting that the Sun, not Earth, was at the universe’s center.
  3. Hershel’s Contribution: In 1805, British astronomer Hershel used a telescope to assert that the solar system is a small part of a galaxy.
  4. Hubble’s Discovery: Edwin P. Hubble (1925) estimated the universe’s diameter to be 2.5 billion light years, consisting of multiple galaxies.

Modern Theories

  1. Big Bang Theory: Proposed by Georges Lemaitre and supported by George Gamow, it suggests that all matter existed in a singular, infinitely dense point, which exploded approximately 15 billion years ago, resulting in the expansion of the universe. Evidence for this theory includes:
    • Cosmic Microwave Background Radiation (CMBR)
    • Wilkinson Microwave Anisotropy Probe (WMAP)
    • Red Shift: Observations that galaxies are moving away, suggesting ongoing expansion.
  2. Red Shift Theory: This theory utilizes the Doppler effect, observing light spectra shifts. When a star moves away, the light shifts toward the red spectrum, indicating the universe’s accelerated expansion.
  3. Steady State Theory: Developed by Bondi, Gold, and Fred Hoyle, it proposes that new galaxies are constantly created as others cross the universe’s boundary, maintaining a constant observable universe size.
  4. Pulsating Theory: Posits an alternating expansion and contraction of the universe. It suggests that gravitational pull could eventually halt expansion, leading to contraction and another explosion, causing pulsation.

Important Note: Recent experiments at the Large Hadron Collider (LHC) aim to recreate post-Big Bang conditions for deeper insights.

Age of the Universe

The age of the universe is approximately 13.7 billion years, based on CMBR measurements. The solar system is estimated to be 4.5 billion years old. The age is calculated by:

  1. Globular Clusters: Dense star collections used for age estimation.
  2. Hubble Constant (Ho): Measures the universe’s expansion rate.

The fate of the universe hinges on the interplay between expansion momentum and gravitational pull. If the density is below a critical level, it will expand indefinitely; if higher, a Big Crunch will occur.

Components of the Universe

The universe is structured in a foamy manner, consisting of filaments, superclusters, and galaxy groups. Visible parts concentrate in certain regions, enclosing vast voids. The universe’s components include:

  1. Dark Energy: Accounts for 68%; influences the acceleration of the universe’s expansion.
  2. Dark Matter: Makes up 27%; detectable through gravitational lensing and galactic dynamics.
  3. Visible Matter: Constitutes only 5%, primarily Hydrogen (72-75%), Helium (23-26%), and other elements (<2%).

Important Note: The visible matter‘s composition has remained relatively constant since the universe’s inception.

Galaxies

A galaxy is a massive star group, existing in diverse sizes and shapes. Key types include:

  1. Normal Galaxies: Emit minimal radio radiation; further categorized as:
  • Elliptical Galaxies: About 18% of galaxies.
  • Spiral Galaxies: Comprise 80%.
  • Irregular Galaxies: Account for 2%.
  1. Radio Galaxies: Emit substantial radio radiation, originating from large radio sources.

The Milky Way, our galaxy, is a spiral type, containing approximately 100 billion stars and a supermassive black hole at its core.

Stars

A star is a luminous body of gases undergoing nuclear fusion. The Sun is our nearest star, taking 8.3 minutes for its light to reach Earth. Stars exist in varying forms:

  1. Single Stars: Only 25% of stars.
  2. Binary Stars: Around 33%, such as Alpha Centauri.
  3. Variable Stars: Show fluctuating luminosity, e.g., Delta Cephei.

Stars like the Sun undergo transformations into red giants, white dwarfs, and potentially black holes depending on their mass.

Concept: The Chandrasekhar Limit states that stars exceeding 1.44 solar masses cannot remain stable as white dwarfs.

Life Cycle of a Star

Stars form in nebulae and undergo several phases:

  1. Protostar formation from collapsing gas and dust.
  2. Transformation into a main sequence star.
  3. Expansion into red giants or red supergiants.
  4. Final collapse leading to white dwarfs, neutron stars, or black holes.

The Solar System

The Solar System is dominated by the Sun, around which eight planets revolve, alongside their satellites, dwarf planets, asteroids, and comets.

The Sun

The Sun forms 99.9% of the Solar System’s mass and is approximately 5 billion years old. It undergoes nuclear fusion, converting hydrogen to helium, producing vast energy.

Concept: The Goldilocks Zone refers to the habitable distance from a star, where a planet’s surface can sustain liquid water.

Planets: Inner and Outer

The Solar System’s planets fall into two categories:

Inner Planets

  1. Mercury: Smallest; closest to the Sun, no atmosphere.
  2. Venus: Similar size to Earth, hottest planet, rotates east to west.
  3. Earth: Has a diverse atmosphere, water, and life.
  4. Mars: Known as the red planet; thin atmosphere with nitrogen and argon.

Outer Planets

  1. Jupiter: Largest, contains 67 satellites, has a Great Red Spot storm.
  2. Saturn: Known for its rings; least dense.
  3. Uranus: Unique tilt; rotates on its side.
  4. Neptune: Discovered through gravitational predictions.

Important Note: Pluto, once the ninth planet, was reclassified as a dwarf planet in 2006.

Comparison of Planets

CategoryInner PlanetsOuter Planets
CompositionRocky surfacesGaseous bodies
MoonsFew or noneMany, often with rings
AtmosphereThin, varied compositionThick, primarily hydrogen and helium

Other Celestial Bodies

Asteroids

Found primarily between Mars and Jupiter, these rocky bodies vary in size. The largest, Ceres, is around 1000 km in diameter.

Comets

Have highly elliptical orbits and display tails when near the Sun. Halley’s Comet appears every 76 years.

Meteors and Meteorites

Small objects entering Earth’s atmosphere, often visible as shooting stars. If they survive entry, they are called meteorites.

Important Note: Meteor showers occur when Earth passes through a comet’s tail.

Recent Discoveries

Exoplanets have been found in systems like TRAPPIST-1, some of which lie in the habitable zone.

MCQ: What accounts for most of the universe’s composition?

  1. Visible matter
  2. Dark matter
  3. Dark energy
  4. Hydrogen

Correct Answer: 3. Dark energy

Home
Notes
Category
My Stuff
Search
Scroll to Top