Cosmic Evolution Project Submenu Links - click to expand or collapse list

                click on underlined bold text to jump to another page






origin of the Universe


cosmic web




Milky Way Galaxy


primordial overdensities

Big Bang


Early cosmic inflation

protons and neutrons

photons and neutrinos

Stars and Galaxies

Solar System






Ice Giants

Trans-Neptunian Objects

Asteroid Belt

Moons and Rings

Earth and Geobiosphere

Global Catastrophes

Ocean Science Quest

Darwin In the Garden

Origin of Life

Diversity of Life

Complexity of Life







Organism Life Cycle

Ecosystem Evolution

Ecosystem Life Cycle

Brains and Tools


Brain Structure

Brain Cell Building Blocks

Brain chemistry and neuroplasticity

Brain Development

Brain Evolution

Brain Emergent Properties


Brain Life Cycle


Tools to expand sensory powers

Tools to expand physical powers

Tools to expand mental powers

Artificial Intelligence

Artificial Selection

Socio-economic Evolution



solar system

The solar system consists of the Sun, Jupiter, Saturn, and a small additional amount of debris which formed all of the other planets, moons, comets, asteroids, etc.

How did the Sun - whose core is extremely hot and dense - form from a cold dilute cloud of gas and dust? What are the vital roles that small amounts of dust play in making life possible in our solar system? Obviously dust is necessary to form rocky planets like Earth as well as the molecules and structures of living things, but dust also affects the lifespan of the Sun.

How is it possible for a giant gas planet like Jupiter to form from the remaining gas and dust beyond the Sun? Was there enough time for Jupiter to form before the Sun ejected the remaining gases from the solar system?


Solar System

The five billion year history of the solar system involves the formation and evolution of the Sun, planets, moons, planetesimals, asteroids, comets, and interplanetary gas and dust. Transformations of energy and matter in the interior of the Sun and planets involve gravitational, electromagnetic and nuclear forces. Heat transport may involve thermal conduction, convection, and radiation. A logarithmic timeline best depicts this domain. NASA image published by

The Sun submenu is a work in progress that will eventually contain slides from ASTR 301 lectures and/or one chapter of an unpublished reference book.

Watch all of these animated gifs from beginning to end

The Jupiter subdirectory contains the slides from an ASTR 301 guest lecture including lecture notes. As a preview, the subdirectory also displays an animated low color resolution gif that runs about four minutes - five seconds for each of the 48 slides.
Venus is often called Earth's twin. Venus has many similarities to Earth, but also many differences. The following animated gif can be downloaded for slower playback. It highlights some of the mysteries hidden below the clouds of Venus.


image from solar system Wikipedia - must add attribution

Ice Giants

image from solar system Wikipedia - must add attribution

Trans-Neptunian Objects

image from solar system Wikipedia - must add attribution

Asteroid Belt

image from solar system Wikipedia - must add attribution

Moons and Rings

image from solar system Wikipedia - must add attribution

The Earth's Moon has its own webpage HERE.

The webpage for the October 10, 2018 Spanos Theatre talk by Amherst College Prof. Kate Follette on her search for exoplanets is at exoplanets.


Accurate Solar System Model made to accurate orbital rotation.

Made with Adobe After Affects and iMovie. Song-
Information on speed of planets comes from Wikipedia Published on Mar 15, 2015 by Jacob Medler 



Back to top



The following pages are excerpts from chapter 2 of my unpublished work-in-progress reference book: - click to expand or collapse

solar and global evolution:

Sun text 01



properties of the Sun








Back to top


Related Content