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Stars
Quick Facts
 
Closest Star to the Earth: Sun
 
Example of a Red Star: Antares
 
Example of a Blue Star: Rigel
 
Hottest Star: Blue Star
 
Coolest Star: Red
 
Color of Our Sun: Yellow
 
Oldest Known Star: Yellow
HE 1523
Stars

Twinkle, twinkle, little star. How I wonder what you are. Well, wonder no more! Stars are large balls of extremely hot gas or, more accurately, hot gas and a gas-like substance called plasma. They are primarily composed of the two most common elements in the universe: hydrogen and helium. The "twinkle" comes from turbulence, or movement, in our atmosphere. It's similar to watching an object from the bottom of the swimming pool; the ripples and movement of the water distort what you see on land. In space, outside of our atmosphere, the stars don't twinkle.

Stars form within clouds of gas, dust, and debris, known as molecular clouds. Read more about the conditions for star formation on our nebulae page. Over the course of billions of years, they pass through several phases and eventually die. (Image Right: White dwarf stars (NASA and H. Richer (University of British Columbia), Courtesy of NASA)

DID YOU KNOW?
Every second, the Sun radiates enough energy to power the entire United States for millions of years.

Cluster of blue stars (Courtesy of NASA)
Features

There are five main characteristics that scientists use to classify stars: brightness, color, surface temperature, size, and mass.

Brightness is described in magnitudes or luminosity. The current scale of magnitude is based on a system invented by the Greek astronomer Hipparchus in approximately 125 B.C. His scale ranged from one (the brightest stars) to six (the faintest). Today, the scale can dip into negative numbers for very bright stars and upwards of twenty for very faint stars.

Even without a telescope, you can see differences in the colors of stars. They range in color from red to yellow to blue. The color is determined by surface temperature. Red stars are the coolest at around 4,040 degrees Fahrenheit, yellow are hotter, and blue are the hottest.

The size of a star is measured in terms of the Sun's radius. So the Sun is one solar radius, while Antares, for example, is 776 solar radii. The Sun's radius is 432,000 miles. Likewise, the mass of a star is measured in comparison to the Sun.

Learn more about star brightness at the Windows to the Universe website.


Chandra X-Ray Observatory (Courtesy of NASA)
Missions

While a number of missions have been sent to study the Sun, we haven't yet sent any missions to other stars. However, missions like the Chandra X-Ray Observatory are expanding our knowledge of the stars from afar.

Launched in the middle of 1999, Chandra was placed outside of the Earth's atmosphere to study x-rays from high-energy regions of the universe, for example, the remains of exploded stars. The observatory is named in honor of Subrahmanyan Chandrasekhar, the late Indian-American Nobel laureate who is widely regarded as one of the top astrophysicists of the twentieth century.

Learn more about Chandra at the mission website.


Ursa Major (Courtesy of NASA)
Myths, Stories, and More

For millennia, humans have been inspired to create stories about the stars. Constellations, the stories of the stars, are numerous and as varied as the cultures on Earth.

One of the most well known constellations is Ursa Major or "Great Bear" in Latin. The back of the "Bear" is often called "The Big Dipper". Unofficial names like these are called, asterisms. Other asterisms for the Great Bear are Plough, Butcher's Cleaver, Charles' Wain (wagon), Northern Dipper, and the Casserole.

Learn how to find the constellations at NASA's Space Place website.


Artist's conception shows a binary-star system where astronomers suspect a Earth-like planet is forming. (NASA/JPL-Caltech)
Earth Matters

Studying stars can tell us a lot about how life formed on Earth. Stars create the key ingredients for life such as carbon, nitrogen, oxygen, and iron. Exploding stars, or supernovae, cast these materials into space and cause new stars to form.

In May of 2008, Chandra's X-Ray Observatory and the National Radio Astronomy Observatory's Very Large Array, discovered the most recent supernova in our galaxy. The supernova explosion occured about 140 years ago. Before that the most recent known explosion was thought to of happened in 1680. Discoveries like these can help us understand how often supernovae explode in the Milky Way Galaxy.

Find out more about this discovery on NASA's Chandra website.

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