Planets around other Stars

Artist's concept of a rocky planet in orbit around a distant star.
Click on image for full size (201 Kb)
NASA, ESA and G. Bacon (STScI)
Did you know that about 200 planets have been discovered in orbit around distant stars? The first planet found to be orbiting a star like our Sun was announced in 1995. Since then astronomers have continued to find new planets outside of our solar system, at a rate of more than one new planet every month!

The star and its planet orbit a common center of gravity. The planet moves in a wide orbit, while the star just appears to wobble slightly. By measuring the Doppler shift from the spectrum of the star, scientists can detect the tiny motion caused by the planet. Most of the distant planets were discovered using this technique.

If we are lucky enough to be lined up properly with the planet's orbit, it can occasionally pass in front of the star, blocking out some of the light that we usually see from the star and briefly making it appear dimmer. It's like a solar eclipse, but the planet only covers a small fraction of the star. Only a few of the planets outside of our solar system pass in front of their stars.

All of the distant planets are much too far away to resolve directly. We can only see their effect on the star that they orbit.


News from NSF: A Newly Discovered Solar System Contains Scaled-Down Versions of Saturn and Jupiter (2/14/08)

Podcasts from NSF: Systemic Search

News from NSF: Small Planet, Small Star (6/2/2008)

Planets around other Stars

Artist's concept of a rocky planet in orbit around a distant star.
Click on image for full size (201 Kb)
NASA, ESA and G. Bacon (STScI)
Did you know that about 200 planets have been discovered around distant stars? The first planet found to be orbiting a star like our Sun was announced in 1995. Since then astronomers have continued to find new planets outside of our solar system, at a rate of more than one new planet every month!

The star and its planet orbit around each other. The planet moves in a wide orbit, while the star just appears to wobble slightly. By measuring the Doppler shift of the light coming from the star, scientists can detect the tiny motion caused by the planet. Most of the distant planets were discovered this way.

If we are lucky, some of the planets can pass in front of their star. This blocks out some of the light that we usually see from the star, briefly making it dimmer. It's like a solar eclipse, but the planet only covers a small part of the star. Only a few planets outside our solar system pass in front of their stars.

All of the distant planets are too far away to see directly. We can only see their effect on the star that they orbit.


News from NSF: A Newly Discovered Solar System Contains Scaled-Down Versions of Saturn and Jupiter (2/14/08)

Podcasts from NSF: Systemic Search

News from NSF: Small Planet, Small Star (6/2/2008)

Planets around other Stars

Artist's concept of a rocky planet in orbit around a distant star.
Click on image for full size (201 Kb)
NASA, ESA and G. Bacon (STScI)
Did you know that about 200 planets have been found around distant stars? The first planet around a star like our Sun was found in 1995. Since then, a new planet has been found almost every month!

The star and its planet move around each other. The planet moves in a wide orbit. The star just wobbles slightly. This causes a Doppler shift of the light. Most of the distant planets were discovered this way.

Some of the planets pass in front of their star. This blocks out some of the light. It makes the star look dimmer. It's like a solar eclipse. The planet only covers a small part of the star. Only a few of the planets pass in front of their stars.

All of the new planets are too far away to see directly. We can only see their effect on the star that they orbit.


News from NSF: A Newly Discovered Solar System Contains Scaled-Down Versions of Saturn and Jupiter (2/14/08)

Podcasts from NSF: Systemic Search

News from NSF: Small Planet, Small Star (6/2/2008)


Page created June 13, 2006 by Travis Metcalfe. Last modified March 13, 2008 by Becca Hatheway.
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