Research

Titan / Project overview

Could a temporary melt pool help assemble life’s ingredients?

An impact can briefly turn Titan’s icy surface into liquid water. I study what chemistry might become possible in that temporary window.

False-color composite of Titan with Selk crater marked by a yellow box.
NASA / JPL / University of Arizona / CNRS / LPG. False-color composite; Selk crater is highlighted.

In brief

What the work suggests

In the reported models, adding a small amount of ammonia opens access to many more of the molecules studied. At 1% ammonia, 38 of the 40 investigated molecules are thermodynamically accessible, compared with five without added ammonia.

Where the evidence stops

Energetic favorability does not establish how quickly reactions happen, how much material survives, or what a spacecraft will find. These calculations offer a chemical baseline to investigate, rather than evidence that life exists on Titan.

The people behind the work

My contribution

I led these two complementary studies with Ben K. D. Pearce at Purdue. Together, they form the first chapter of my PhD: a shared thermodynamic view of amino acids, nucleobases, ribose, and fatty acids in a Titan-like melt pool.

The approach

Turning a question into calculations

We start with water and simple organic ingredients, then calculate which molecular arrangements are energetically favored. By varying the starting amount of ammonia, we ask how the accessible chemical inventory changes.

One ingredient, a very different chemical picture

Ammonia changes the supply of hydrogen available to build molecules. The interactive lets you step through the reported starting concentrations and see how the modeled molecular inventory changes.

See the ideas take shape

Step inside the science.

Follow the setting, explore the model, and take a closer look at the evidence. Technical explanations are there when you want them.

Explore Titan

An open question

How closely can real melt-pool chemistry approach these modeled outcomes, and what traces might remain for Dragonfly to investigate?

Go to the source

Papers & related resources

  1. 2026

    Prebiotic Chemistry Insights for Dragonfly. II. Thermodynamic Favorability of Nucleobases, Ribose, and Fatty Acids in Selk Crater on Titan (opens in a new tab)

    Ishaan Madan & Ben K. D. Pearce · The Planetary Science Journal 7, 107

  2. 2025

    Prebiotic Chemistry Insights for Dragonfly: Thermodynamics of Amino Acid Synthesis in Selk Crater on Titan (opens in a new tab)

    Ishaan Madan & Ben K. D. Pearce · The Planetary Science Journal 6, 284

AbSciCon · 2026

Prebiotic Chemistry Insights for Dragonfly

Thermodynamics of amino acid, nucleobase, ribose, and fatty acid synthesis in Selk crater on Titan.

For curious readers & researchers · Slides

View slides (opens in a new tab)

Telluride Science · 2025

Alternative Chemistries Beyond Earth

Venusian heteropolymers and Titan’s amino acids.

For curious readers & researchers · Slides

View slides (opens in a new tab)

A personal connection

This work brought together the chemistry, computation, and planetary questions that drew me back to research after working in healthcare software.

Read that part of my story