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Earth Science Regents Review Essentials

May 17, 2025

Earth Science New York State Regents Review - Part 1

Introduction

  • Presenter: Donnie Rudansky
  • Course: Earth Science New York State Regents by Regents Made Simpler
  • Importance of familiarity with the 16-page reference table as many questions are based on it.

Reference Table Overview

Key Equations on Page 1

  • Rate of Change:

    • Formula: Change in value over time.
    • Example: Calculate temperature change from 8 a.m. to 2 p.m.
    • Calculation: From 24°C to 15°C over 6 hours = 1.5°C per hour.
  • Density:

    • Formula: Density = Mass / Volume.
    • Example: 22 grams in 5 cubic cm = 4.4 g/cm³.

The Universe and Big Bang Theory

  • Origin: Universe began 14 billion years ago with the Big Bang.
  • Hydrogen Atoms: First atoms forming stars and galaxies.

Gravity and Nuclear Fusion

  • Gravity: The force causing hydrogen atoms to cluster and form stars through nuclear fusion.
  • Nuclear Fusion: Process where hydrogen atoms collide to form stars.

Galaxies

  • Formed by clusters of stars.
  • Types:
    • Spiral, Irregular, Elliptical.

Evidence for Big Bang

  • Cosmic Background Radiation: Residual radiation from the Big Bang.
  • Doppler Effect: Redshift in galaxies indicating expansion.

Life Cycle of Stars

  • Characteristics:
    • Luminosity, Surface Temperature, Color.
  • Stages:
    • Main Sequence, Giant/Supergiant, White Dwarf, Neutron Star, Black Hole.

Our Solar System

Formation

  • Formed 4.6 billion years ago.
  • Heliocentric Model: Planets orbit around the Sun, not Earth.

Planets

  • Terrestrial Planets: Mercury, Venus, Earth, Mars (rocky, higher density).
  • Jovian Planets: Jupiter, Saturn, Uranus, Neptune (gas giants, lower density).
  • Asteroid Belt: Between Mars and Jupiter.

Eccentricity and Orbits

  • Planets have elliptical orbits, affecting speed of revolution.
  • Eccentricity: Measure of how much an orbit deviates from a circle.

Earth's Rotation and Revolution

Evidence for Earth's Motion

  • Revolution:

    • Different constellations visible throughout the year.
    • Seasonal changes due to Earth's orbit around the Sun.
  • Rotation:

    • Foucault Pendulum: Evidence of Earth rotating on its axis.
    • Coriolis Effect: Wind patterns due to Earth’s rotation.

Earth's Seasons

Causes of Seasons

  • Axial Tilt: Earth is tilted at 23.5°.
  • Sun’s rays: Angle and duration of insolation affects temperature.

Seasonal Changes

  • Winter Solstice: December 21st, Northern Hemisphere tilted away.
  • Spring Equinox: March 21st, rays hit directly at the equator.
  • Summer Solstice: June 21st, Northern Hemisphere tilted towards the Sun.
  • Fall Equinox: September 21st, rays hit directly at the equator.

Conclusion

  • Course Details: Available for $89, covering simplified review and video explanations.
  • Additional Offerings: Includes visuals from past Regents exams.

For more information, visit Regents Made Simpler.