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The Wall Street Publication > Blog > Tech > How Do Astronomers Discover Planets in Different Photo voltaic Methods?
Tech

How Do Astronomers Discover Planets in Different Photo voltaic Methods?

Editorial Board Published December 14, 2025
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How Do Astronomers Discover Planets in Different Photo voltaic Methods?
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It was nearly 100 years in the past that Clyde W. Tombaugh found Pluto. That was the final planet discovered till 1992, when people discovered one other one. However this new planet wasn’t in our photo voltaic system—it was orbiting one other star. We name this an extrasolar planet, or “exoplanet” for brief.

Since then, astronomers have cataloged greater than 6,000 exoplanets. Should you thought it was exhausting to recollect the names of our personal planets, strive all of the planets, with names like HD 189733b. (A jolly place the place it rains molten glass and the wind blows 9,000 kilometers per hour.)

Even the closest exoplanets are greater than 4 mild years away (36 trillion miles), which makes it uncertain that we’ll ever go to one—so why hassle? The reason being, it helps us reply an age-old query: Are we alone within the universe? So far as we perceive, you want a planet to have life, and the race is on to find one with Earth-like qualities.

Why Are They Onerous to Discover?

The issue is, you possibly can’t simply take your greatest telescope and begin trying across the sky. Telescopes have a restricted resolving energy—the smallest angular measurement they’ll “see.” For the Hubble House Telescope that’s 0.05 arc second, which is extremely tiny—about 1/72,000th of a level. The HST may make out a large, Jupiter-size planet at a distance of 590 billion kilometers. That’s superb, but it surely’s simply 0.06 mild yr, and the closest star, Proxima Centauri, is 4.25 mild years away.

One other downside is the dimness of planets. Certain, Jupiter is simple to see in our personal evening sky, due to the daylight reflecting off its floor. However you possibly can’t see Jupiter in any respect throughout the day, as a result of that mirrored mild is way dimmer than direct daylight. It’s the identical for exoplanets. After we’re trying on the mild from a star, the planets round it simply aren’t vibrant sufficient to be discernable.

Fortunately, there are different strategies, and I’m going to elucidate the 2 that had been used to search out many of the exoplanets we all know at present. There is a bunch of cool physics right here, so let’s go!

Orbits, Jiggly Stars, and Blue Shifts

What occurs when a planet strikes round a star? First, there’s a gravitational interplay that pulls the planet within the course of the star. The magnitude of this pressure (FG) is determined by the mass of the star (M) and the planet (m), in addition to the space (r) between them:

Image may contain Stencil

Illustration: Rhett Allain

TAGGED:astronomersfindplanetsSolarSystems
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