Dimitri Veras

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Associate Professor & STFC Ernest Rutherford Fellow

University of Warwick

United Kingdom

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About

Dimitri Veras is an Associate Professor and STFC Ernest Rutherford Fellow at the University of Warwick, UK. His research primarily focuses on the dynamics and characteristics of planetary systems, particularly in relation to white dwarfs and the formation of extrasolar planetesimals. Recent articles by Professor Veras explore topics such as the resupplying of planetary debris and the disruption of exo-asteroids, contributing significantly to the understanding of minor planets and their environments.

Recent Grants

Grant: Close

Impact of solar storms and space weather on tracking capabilities of satellites and destructive debris

Open Date: 2022-07-01

Close Date: 2023-12-01

Grant: Close

State change detection and shape analysis of space debris

Open Date: 2021-12-01

Close Date: 2022-03-01

Grant: Close

Pressing Challenges in Post-Main-Sequence Planetary Science

Open Date: 2017-09-30

Close Date: 2022-09-29

Grant: Close

Using moons to explain observations of rocky pollutants in white dwarfs

Open Date: 2014-11-01

Close Date: 2015-11-01

Articles (21)

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2022

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2022

Collaborators (15)

Mia Sloth Lundkvist

Aarhus University

DENMARK

Dimitri Veras

Research Interests

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About

Recent Grants

Articles (21)

Discovery of an icy and nitrogen-rich extrasolar planetesimal

Disc–planet misalignment from an unstable triple system: IRAS04125

Bounding destruction time-scales of minor planets orbiting white dwarfs with the sesquinary catastrophe

Resupplying planetary debris to old white dwarfs with supernova blast waves

The dearth of high-mass hydrogen-atmosphere metal-polluted white dwarfs within 40 pc

Characterizing planetary material accreted by cool helium-atmosphere white dwarfs using an exponentially decaying disc model

Dynamics of Two Planets near a 2:1 Resonance: Case Studies of Known and Synthetic Exosystems on a Grid of Initial Configurations

Constraints on Remnant Planetary Systems as a Function of Main-sequence Mass with HST/COS

Forming planetary systems that contain only minor planets

Disruption of exo-asteroids around white dwarfs and the release of dust particles in debris rings in co-orbital motion

TESS Asteroseismic Analysis of HD 76920

Planetesimals drifting through dusty and gaseous white dwarf debris discs: Types I, II and III-like migration

A close-in giant planet escapes engulfment by its star

Survival and dynamics of rings of co-orbital planets under perturbations

Constellations of co-orbital planets: horseshoe dynamics, long-term stability, transit timing variations, and potential as SETI beacons

Binary asteroid scattering around white dwarfs

TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars

The smallest planetary drivers of white dwarf pollution

On the orbital decay of the gas giant Kepler-1658b

High-resolution resonant portraits of a single-planet white dwarf system

Mathematical encoding within multiresonant planetary systems as SETI beacons

Collaborators (15)

Mia Sloth Lundkvist

Ian Dobbs-Dixon

David Kipping

Hossam Aly

Adina D Feinstein

Jakob Lysgaard Rørsted

Adrian Barker

Pier-Emmanuel Tremblay

Tim Bedding

Jeremy Smallwood

Andre Izidoro

Yaguang Li

Amalie Stokholm

Matthew Clement

Jamie Williams

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