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How to find a planet you can’t see
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Tiny wobbles and faint twinkles that have led astronomers to nearly 5,000 new worlds.
So when astronomers set out to search for planets around other stars (aka “exoplanets), they knew it wouldn’t be easy. Our closest neighbor, a little red dwarf named Proxima Centauri, is 7,000 times further away from us than Pluto. Any planets in orbit around it would likely get lost in the glare of bright starlight.
“Trying to see an earthlike planet across interstellar distances,” writes astrophysicist Adam Frank, “would be like looking from New York City to AT&T Park in San Francisco, where the Giants play, and making out a firefly next to one of the stadium spotlights.”
“To detect or study an exoplanet,” says Sara Seager, a planet-hunting astrophysicist at MIT, “we have to work with the star.”
Astronomers started monitoring stars for tiny changes that could hint at the presence of one or more planets. Early efforts focused on the search for a wobble. The pull of a planet’s gravity causes a star to circle their mutual center of gravity - and from our vantage point the star seems to swing back and forth. In 1995, a Swiss team picked up the signature of just such a wobble in the starlight from a yellow dwarf in the Pegasus constellation. They had found 51-Pegasi b: the first exoplanet around a sun-like star.
Fifty years ago, astronomers had no idea what percentage of stars had planets. A common educated guess was 20%, but for all we knew it could have been zero. But based on what we’ve seen since, it seems possible that every star has at least one planetary companion.
Now that we know exoplanets exist, it’s time to learn more about them. What are they made of? How did they form? And, most tantalizing, could they harbor life? We’re like sailors who have spotted a tiny rise of land on the horizon. Now we want to study this new island’s geology and biology and make contact with any inhabitants … but we have to do it all from aboard our ship, floating trillions of miles out at sea.
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Presented by the Center for Matter at Atomic Pressures (CMAP) at the University of Rochester,
a National Science Foundation (NSF) Physics Frontier Center, Award PHY-2020249
Any opinions, findings, conclusions, or recommendations expressed in this material are those of the authors and do not necessarily reflect those of the National Science Foundation.
~~~
Further reading:
The discovery of 51 Pegasi b:
The potential of the James Webb Space Telescope
The Smallest Lights in the Universe - Sara Seager’s memoir
Light of the Stars: Alien Worlds and the Fate of the Earth
The fraught and fractious history of failed exoplanet discoveries:
So when astronomers set out to search for planets around other stars (aka “exoplanets), they knew it wouldn’t be easy. Our closest neighbor, a little red dwarf named Proxima Centauri, is 7,000 times further away from us than Pluto. Any planets in orbit around it would likely get lost in the glare of bright starlight.
“Trying to see an earthlike planet across interstellar distances,” writes astrophysicist Adam Frank, “would be like looking from New York City to AT&T Park in San Francisco, where the Giants play, and making out a firefly next to one of the stadium spotlights.”
“To detect or study an exoplanet,” says Sara Seager, a planet-hunting astrophysicist at MIT, “we have to work with the star.”
Astronomers started monitoring stars for tiny changes that could hint at the presence of one or more planets. Early efforts focused on the search for a wobble. The pull of a planet’s gravity causes a star to circle their mutual center of gravity - and from our vantage point the star seems to swing back and forth. In 1995, a Swiss team picked up the signature of just such a wobble in the starlight from a yellow dwarf in the Pegasus constellation. They had found 51-Pegasi b: the first exoplanet around a sun-like star.
Fifty years ago, astronomers had no idea what percentage of stars had planets. A common educated guess was 20%, but for all we knew it could have been zero. But based on what we’ve seen since, it seems possible that every star has at least one planetary companion.
Now that we know exoplanets exist, it’s time to learn more about them. What are they made of? How did they form? And, most tantalizing, could they harbor life? We’re like sailors who have spotted a tiny rise of land on the horizon. Now we want to study this new island’s geology and biology and make contact with any inhabitants … but we have to do it all from aboard our ship, floating trillions of miles out at sea.
~~~
Presented by the Center for Matter at Atomic Pressures (CMAP) at the University of Rochester,
a National Science Foundation (NSF) Physics Frontier Center, Award PHY-2020249
Any opinions, findings, conclusions, or recommendations expressed in this material are those of the authors and do not necessarily reflect those of the National Science Foundation.
~~~
Further reading:
The discovery of 51 Pegasi b:
The potential of the James Webb Space Telescope
The Smallest Lights in the Universe - Sara Seager’s memoir
Light of the Stars: Alien Worlds and the Fate of the Earth
The fraught and fractious history of failed exoplanet discoveries:
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