There are many ingredients for life in the Universe. The goal of modern astronomy and planetary science is to detect life beyond Earth.

Two scientists are studying exoplanets and Astrobiology. Researchers like us will soon be able to measure the chemical makeup of atmospheres of planets around other stars thanks to next- generation telescopes.

One or more of these planets may have a chemical signature of life.

Habitable exoplanets

There could be life in the Solar System if there is liquid water. It's difficult to find life in these places as they are hard to reach, and it would take a probe to detect life.

It's possible that life will first be found on a planet in the vicinity of a star.

There are around 300 million potentially habitable planets in the universe alone and many of them are Earth-sized planets.

Over 5,000 exoplanets have been discovered using indirect methods that measure how a planet affects its nearby star. Astronomers can get information on the mass and size of an exoplanet, but it's not much.

Looking for biosignatures

Astrobiologists use starlight to detect life on distant planets. The light may carry a clue if the atmosphere was changed by life.

Earth had an atmosphere without oxygen for the first half of it's existence. The biosignature of Earth was very faint. A new family of algae was the cause of the change.

The oxygen produced by the process of photosynthesis is free of bonds to other elements. The biosignature on light that passes through it has been left by Earth's oxygen filled atmosphere.

The light's wavelength is more likely to be trapped in the gas or material's surface when it bounces off. There is a reason objects are different colors.

The leaves are green because of their ability to absorb light. Most of the green light bounces back into your eyes after hitting a leaf.

The composition of the material that the light interacts with determines the pattern of missing light. Calculating the specific color of light that comes from a planet can be used to determine the composition of an exoplanet's atmosphere or surface.

This method can be used to recognize the presence of certain atmospheric gases that are associated with life, such as oxygen or methane. It is possible to detect strange colors on a planet.

Plants and algae use the chlorophyll and other pigments to capture the light's wavelength.

The characteristic colors that can be detected are produced by these pigments. It is possible to see this color reflecting off the surface of a distant planet.

Telescopes in space and on Earth

There are subtle changes to the light coming from a potentially habitable exoplanet. The only telescope capable of such a feat is the new james wbb space telescope

JAMES WADD took a reading of the spectrum of the gas giant exoplanet WASP-96b. Water and clouds were visible in the spectrum, but WASP-96b is not likely to host life.

The data shows that James is able to detect faint chemical signatures in light.

TRAPPIST-1e is a planet that is 39 light-years from Earth and is set to be turned into a mirror by the end of the year.

As planets pass in front of their host stars and capture starlight that filters through the planet's atmosphere, Webb can look for biosignatures. The telescope is only able to look at a few of the closest potentially life-supporting worlds.

Carbon dioxide, methane, and water Vapor can only be detected by it. The strongest signal for life is the presence of unbonded oxygen.

Plans to block the bright light of a planet's host star to reveal starlight reflected back from the planet are one of the leading concepts for the future. The idea is similar to using your hand to block the sun's rays.

Small, internal masks or large, external, umbrella-like spaceships could be used to do this. It's easier to study light bouncing off a planet once the starlight is blocked.

Three enormous, ground-based telescopes are currently under construction that will be able to look for biosignatures.

Even though Earth's atmosphere distorts starlight, these telescopes may be able to probe the atmospheres of the closest worlds for oxygen.

Is it biology or geology?

Astrobiologists will only be able to detect biosignatures from worlds that have been completely transformed by life, even with the most powerful telescopes of the future.

Most gases released by life can be produced by nonbiological processes. When sunlight splits water into oxygen and hydrogen, it also creates oxygen.

Astronomers can detect false positives if they understand a planet well enough.

The next generation of exoplanet studies has the ability to prove the existence of life. The first data release from the space telescope gives us a glimpse of what's to come.

Chris Impey is a professor of astronomy at the University of Arizona.

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