Inferring Planet and Disk Parameters from Protoplanetary Disk Images Using a Variational Autoencoder

TL;DR

This paper introduces VADER, a variational autoencoder framework that infers planet and disk parameters from protoplanetary disk images, achieving high accuracy and efficiency, and validated on synthetic and real ALMA data.

Contribution

The paper presents the first VAE-based method for inferring multiple planet and disk parameters from dust continuum images, with full posterior distributions and rapid inference capabilities.

Findings

VADER accurately recovers planet masses with R^2 > 0.9.

Reconstructed disk morphologies have high structural similarity (>0.99).

Inferred parameters from real images are consistent with literature.

Abstract

Dust-continuum observations of many protoplanetary disks reveal rings and gaps that are widely interpreted as evidence of ongoing planet formation. Here we present the first framework for inferring planet and disk parameters from such images using variational autoencoder (VAE) based generative machine learning (ML). The new framework is called VADER (Variational Autoencoder for Disks with Embedded Rings). We train VADER on synthetic images of dust continuum emission, generated from \texttt{FARGO3D} hydrodynamic simulations post-processed with Monte Carlo radiative transfer calculations. VADER infers the masses of up to three embedded planets as well as the disk parameters viscous $\alpha$, dust-to-gas ratio, Stokes number, and flaring index. VADER returns a full posterior distribution for each of these quantities. We demonstrate that VADER reconstructs disk morphologies with high structural similarity (index $>$ 0.99), accurately recovers planet parameters with $R^2 > 0.9$ across planet masses, and reliably predicts disk parameters. Applied to ALMA dust continuum images of 23 protoplanetary disks, our model returns mass estimates for embedded planets of 0.3-2~$M_{\mathrm{Jup}}$ that agree to within $1\sigma$ of published values in most cases, and infers disk parameters consistent with current literature. Once trained, the VAE performs full posterior parameter inference in a matter of minutes, offering statistical rigor with enough computational speed for application to large-scale ALMA surveys. These results establish VAE-based models as powerful tools for inferring from disk structure the masses of embedded planets and the global disk parameters, with their associated uncertainties.