Portrait of Dmitry Semenov
Astrophysics · Astrochemistry · Planet Formation
Heidelberg, Germany · Max Planck Institute for Astronomy / Heidelberg University

Dmitry
Semenov

I study how chemistry evolves from molecular clouds to planet-forming disks — and how the molecular inventory of young planetary systems may connect to the origins of prebiotic chemistry.

Max Planck Institute for Astronomy · Heidelberg
Astrochemistry · disks · molecular observations
Models, networks & data products
Teaching at Heidelberg University
V883 Ori abundance map frame A V883 Ori abundance map frame B V883 Ori abundance map frame C V883 Ori abundance map frame D V883 Ori abundance map frame E
V883 OriFrame A / very early
Time-dependent abundances after the outburst begins
A→E follows the early-to-late chemical evolution sequence in the V883 Ori disk.
01 / About

From molecules
to planetary systems.

I am a guest scientist at the Max Planck Institute for Astronomy in Heidelberg and a senior post-doc researcher at the ZAH / Institute for Theoretical Astrophysics at Heidelberg University.

My work combines astrochemical modeling with infrared and radio observations to understand the physical and chemical evolution of star-forming regions and protoplanetary disks.

I develop numerical models and tools for disk chemistry, reaction networks, and observational interpretation, with a particular interest in complex organic molecules and chemical inheritance.

“Astrochemistry and planet formation lie at a crossroad between molecular astrophysics, planetary science, and the origin of life.”
02 / Research

Four key questions
drive my scientific work.

Coupled evolution of matter, radiation, and chemistry during the formation of stars and planetary systems.

01

Planet-forming disks

Chemical evolution of the solar nebula and protoplanetary disks, including the physical processes controlling molecular abundances and distributions.

02

Isotopic & dust grain chemistry

Isotopic fractionation, surface chemistry, ice evolution, and the chemical inheritance of forming planetary systems.

03

Molecular observations

Interferometric and single-dish observations at (sub-)millimeter wavelengths and the interpretation of molecular emission as a diagnostic of disk physics and chemistry.

04

Organic chemistry & origins

Formation and evolution of simple and complex organic molecules in space and their possible links to prebiotic chemistry.

03 / Scientific tools

Models, networks,
& data products.

Reduced network

Rednet

Reduced reaction network for modeling ionization and chemistry in disks.

Rednet →
Dust & radiative transfer

Optical constants

The Heidelberg–Jena Database of Optical Constants for astrophysical materials.

Opacity database →
04 / Career & research timeline

Two decades of astrochemistry
and planet-formation research.

A compact view of the main stages in my research career, teaching, grants, and community activity.

2000–2005

PhD · Friedrich Schiller University Jena

Doctoral work on dust and gas in protoplanetary discs.

PhD awarded in 2005 · supervisor: Thomas Henning
2005–2017

MPIA · Planet and Star Formation

Postdoctoral research on disk chemistry, astrochemical modeling, molecular observations, and the development of ALCHEMIC.

Granted PI observing time at IRAM/PdBI/NOEMA and later ALMA.
2012–present

Molecular Astrophysics · Heidelberg University

Annual lecture course in molecular astrophysics and astrochemistry.

Teaching with Holger Kreckel and collaborators.
2018

Cozzarelli Prize · PNAS

Co-recipient of the Cozzarelli Prize for one of the best PNAS articles of 2017.

2018–2025

MPIA · Planet and Star Formation

Research on protoplanetary-disk physics and chemistry, large observing programmes, supervision, and international collaborations.

2025–2028

DFG project · Protoplanetary disks in the era of JWST and ALMA

Principal investigator of an individual DFG grant focused on the new observational era for planet-forming disks.

SE 1962/7-1
2025–present

Institute for Theoretical Astrophysics · Heidelberg University

Continuing research on astrochemistry, disk evolution, and molecular diagnostics while maintaining close links with MPIA.

06 / Selected papers

A few highlighted papers

2026A&Aplanet formation

AB Aur, a Rosetta stone for studies of planet formation

A recent study framing AB Aur as a key system for understanding multiple facets of disk structure and planet formation.

2026A&Amolecular clouds

The converging gas flow around the infrared dark cloud G28.37

A recent example of work connecting physical gas flows, structure formation, and chemically relevant environments.

librarycuratedfull list

Complete scientific library

Your public NASA ADS library remains the canonical destination for the full, current, and curated publication record.

07 / Latest papers

Latest publications,
updated automatically.

This feed queries Crossref for works registered with my ORCID and sorts them by publication date. Because ORCID metadata are not present in every publisher deposit, my public NASA ADS library remains the complete bibliography.

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08 / Teaching

Molecular astrophysics
from theory to observation.

Together with PD Dr. Holger Kreckel (MPIK) and Dr. Caroline Gieser (MPIA), I teach astrochemistry and molecular astrophysics at Heidelberg University, with course material covering the physics, chemistry, and observational diagnostics of molecules in space.

9 / Contact

Let's talk science.

Ruprecht-Karls-Universität Heidelberg · Zentrum für Astronomie · Institut für Theoretische Astrophysik · Albert-Ueberle-Str. 2 · 69120 Heidelberg · Germany

Office 006B+49 (0) 6221 / 54-6712dmitry.semenov@uni-heidelberg.de

Max Planck Institute for Astronomy · Königstuhl 17 · 69117 Heidelberg · Germany

Office I-120+49 (0) 6221 528-354semenov@mpia.de