Where are stars born? Are stars being born right now?
Stars are born in clouds like the one in the picture. Gravity pulls material together. When it is extremely dense, it begins nuclear fusion. That is, it becomes a star. We can see places where stars are being born right now. Of course, it takes light a long time to travel to us. So what we see right now may have happened many millions or even billions of years ago.
Formation of the Solar System
Our solar system began about 5 billion years ago. The Sun, planets, and other solar system objects all formed at about the same time. The leading hypothesis for how they formed is called the
The Solar Nebula
The Sun and planets formed from a giant cloud of gas and dust. This was the
. The cloud contracted and began to spin. As it contracted, its temperature and pressure increased. The cloud spun faster and formed into a disk. Scientists think the solar system at that time looked like these disk-shaped objects in the Orion Nebula. New stars are forming in the Orion Nebula today.
Solar System Bodies Form
Gravity pulled a lot of material to the center of the cloud. Temperatures and pressures at the center of the cloud were extreme. It was so hot that
reactions began. A star was born—the Sun. In these reactions, hydrogen fuses to make helium. Extreme amounts of energy are released.
An artist’s painting of a protoplanetary disk.
Meanwhile, the outer parts of the disk were cooling off. Matter condensed from the cloud. Small pieces of dust started clumping together. These clumps collided and combined with other clumps. Gravity brought more clumps together to make larger bodies. Gravity at the center of the disk attracted rock and metal. Lighter material remained farther out in the disk. Eventually, these small bodies grew to become the planets and moons that we find in our solar system today.
Since gravity pulled the heavy material inward, the inner planets—Mercury, Venus, Earth, and Mars—are made of rock and metal. The outer planets—Jupiter, Saturn, Uranus, and Neptune—condensed farther from the Sun (
). They are made from lighter materials such as hydrogen, helium, water, ammonia, and methane. Out by jupiter and beyond, where it’s very cold, these materials form solid particles. Dwarf plants, comets, and asteroids formed too.
The Sun and planets (note that this image is old enough to include Pluto, which is no longer considered one of the planets).
The nebular hypothesis explains the basic features of the solar system:
The orbits of the planets lie in nearly the same plane. The Sun is at the center.
The planets revolve in the same direction.
The planets mostly rotate in the same direction.
The axes of rotation of the planets are mostly nearly perpendicular to the orbital plane.
The oldest Moon rocks are 4.5 billion years old.
This video, from the ESA, discusses the Sun, planets, and other bodies in the solar system and how they formed. The first part of the video explores the evolution of our view of the solar system starting with the early Greeks who reasoned that since some points of light—which they called planets—moved faster than the stars, they must be closer:
The center of the nebula became a star, our Sun!
A giant cloud of dust and gas is called a nebula. A nebula collapsed to form the solar system. This is the nebular hypothesis.
When hydrogen began to fuse into helium, the Sun became a star.
Planets nearer the Sun are formed of denser metal and rocks. Planets farther out are lighter and gaseous.
Use the resource below to answer the questions that follow.
What is a protostar?
At what temperature did nuclear fusion begin?
When was our star born? How much longer will it last?
How does the Sun produce its light?
What does recent research suggest about the birth of our Sun?
What was the Big Bang?
What is the nebular hypothesis?
What was the solar nebula?
How did the material at the center of the solar system become a star?
What are the categories of bodies in the solar system? In general, where can they be found?
What is the evidence that supports the nebular hypothesis?