Making planets

Exoplanet research is fundamentally about understanding the diverse ways that worlds are constructed and how they evolve within their stellar environments. By analyzing the chemistry and physics of these extreme alien worlds, we can determine where a planet was born and uncover the universal mechanisms that govern planetary formation.
Hannah Wakeford

Associate Professor of Astrophysics

07 May 2026
Hannah Wakeford
Citation-ready summary

Exoplanet research is fundamentally about understanding the diverse ways that worlds are constructed and how they evolve within their stellar environments. By analyzing the chemistry and physics of these extreme alien worlds, we can determine where a planet was born and uncover the universal mechanisms that govern planetary formation.

Author: Hannah Wakeford
Last updated: 07 May 2026
Key Points
  • Exoplanets, which orbit stars other than our Sun, come in architectures vastly different from our own, such as "hot Jupiters" that orbit their stars in under a week.
  • The most common type of planet in our galaxy is a size between Earth and Neptune—an example that does not exist within our own solar system.
  • Measuring an exoplanet's atmosphere through transits allows scientists to identify chemical markers like methane and water vapor, which reveal where the planet was born.
  • The discovery of "missing water" in many exoplanet atmospheres was solved by the realization that clouds were masking the chemical signatures scientists were trying to measure.

New planetary systems

Exoplanets are planets that orbit stars other than our Sun, so they're outside of our solar system. The first exoplanet orbiting a sun-like star, discovered in 1995, is called 51 Pegasi b. This discovery completely changed the way we look at our solar system and the possibilities of the universe. This planet orbits its star in under a week. It is the size of Jupiter, about 11 times the radius of Earth, but orbits 20 times closer to its star than we are to the Sun.

© NASA

We have these small, rocky planets close to our star and gas giants like Jupiter farther away. This system was a gas giant right next to its star, and the rocky planets were nowhere to be seen. This requires us to understand that our neat configuration might not be the most common way planetary systems are structured. Thousands more detections have shown that the architecture and configuration of giant and small planets is very different than our own and comes in a huge variety of ways.

Sub-Neptunes and Super-Earths

The most common size of exoplanet in our galaxy is non-existent in our solar system. These planets are sub-Neptune in size. Neptune is the smallest of our gas giants, sitting at the furthest distance from our Sun and mostly made of hydrogen and helium. Earth is the largest rocky planet in our system. About 50% of discovered planets are actually somewhere between the size of Earth and Neptune. The big question this poses is what they are made of: are they super-sized rocks, called super-Earths, or compressed gas giants, called mini-Neptunes?

Artist's conception of a mini-Neptune or "gas dwarf" © Wikimedia

What are their atmospheres made of?

From the discovery of 51 Pegasi b, a hot Jupiter sitting right next to its star and heated by radiation, to the Kepler mission showing a galaxy filled with super-Earths, we have a fundamental question: what are their atmospheres made of? An atmosphere defines the environment and where a planet formed in the first place.

Artist impression of a small, rocky planet transiting across the face of its parent star. © ESA

If a giant planet is close to its star, it did not form there because there is not enough material that close to a forming star. It had to have moved through its planetary system, potentially destroying other planets or changing its atmospheric composition along the way. A transiting planet allows us to measure its atmosphere.

How planets are born

We expect to discover atmospheres dominated by hydrogen and helium, which are hard to measure. We look for tiny components, such as water vapor, CO2, and methane. The relationship between carbon monoxide and methane can tell us a huge amount about the chemical and thermal structure of an atmosphere.

Helium-Shrouded Planets (Artist's Concept) © Wikimedia

These measurements inform us about where a planet was born. Was it born close to the star, or farther away where ices start to freeze out? If it formed in a region where water becomes solid, it will be water-dominated. Further out, it will be dominated by carbon species that freeze at colder temperatures. Atmospheric materials tell us where a planet formed, helping us understand how easy it is to make a planet.

The mystery of missing water

Very early on, we used the Hubble Space Telescope to look for water vapor, which is one of the most common molecules in the entire universe. We find it orbiting black holes, in star formation regions, and across our solar system. We expected water to be mixed within these atmospheres, but we found less than expected.

Clouds surrounding the exoplanet Kepler-7b © NASA

This opened the question of whether these planets formed in dry environments or if something in the atmosphere was blocking the signatures. It turns out something was obscuring the light as it passed through, preventing us from measuring the full extent of water absorption. Those features were being masked by clouds.

Community discovery

The study of exoplanets requires a whole team of scientists together to make discoveries. The amazing diversity of worlds requires different questions and techniques. Our communities require experts in observations, data analysis, stars, and chemists to understand alien chemical networks. Science isn't done on its own anymore, and exoplanets is a perfect field to show how community comes together.

© NASA

Looking for aliens

If I was to single out one misconception in the field, it is that we're all looking for aliens. What we're looking for is understanding about how these planets are made and how the dynamics of a system might change the way a world sees the universe. We want to fundamentally understand the physics, chemistry, and mechanisms behind these extreme environments; it is not always about aliens.

Grey Aliens Drawing © Wikimedia

Editor’s note: This article has been faithfully transcribed from the original interview filmed with the author, and carefully edited and proofread. Edit date: 2026

Discover more about

Making planets

Wakeford, H R, Sing, D K, Stevenson, K B et al, (2020), Into the UV: A Precise Transmission Spectrum of HAT-P-41b Using Hubble's WFC3/UVIS G280 Grism. The Astronomical Journal, , Volume 159, Issue 5, id.204, 15 pp.

Wakeford, H R, Wilson, T J, Stevenson, K B, Lewis, N K, (2019), Exoplanet Atmosphere Forecast: Observers Should Expect Spectroscopic Transmission Features to be Muted to 33%. Research Notes of the American Astronomical Society, Volume 3, Issue 1, article id. 7.

Wakeford, H R, Lewis, N K, Fowler, J, Bruno, G et al, (2019), Disentangling the planet from the star in late type M dwarfs: A case study of TRAPPIST-1g. The Astronomical Journal, Volume 157, Issue 1, article id. 11, 14 pp.

Sing, D.K, Fortney, J.J, Nikolov, N., Wakeford, H.R. et al, (2015), A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion. Nature 529, 59–62 (2016).

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