A Preliminary Search for Planets and Exozodiacal Emission Around <i>α</i> Centauri A with JWST/MIRI

Abstract We present F1550C (15.5 μ m) coronagraphic imaging observations of the nearest solar-type star α Cen A using the James Webb Space Telescope (JWST) Mid-InfraRed Instrument (MIRI). The observations, executed in 2025 February, were compromised by having only one successful roll and degraded performance due to a position mismatch (Δ r ∼ 10 mas) between α Cen A and the best-matching reference observation behind the MIRI coronagraph. We set preliminary upper limits on both the presence of a planet and an exozodiacal dust disk. The observations are sensitive to a planet heated by α Cen A (200–250 K) with a radius ≳1 R Jup at a separation of 1 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>.</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>″</mml:mi> </mml:mrow> </mml:mover> </mml:math> 5 (2 au) and zodiacal dust emission at the level of ≳5–10 times the brightness of our own zodiacal cloud. A complete analysis of all JWST/MIRI observations of α Cen A is forthcoming in Paper I (Beichman &amp; Sanghi et al. 2025, in preparation) and Paper II (Sanghi &amp; Beichman et al. 2025, in preparation).

Authors

Publication Details

Journal
Research Notes of the AAS
Published
2025-05-16
DOI
https://doi.org/10.3847/2515-5172/add880
Citations
2
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
2.31
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

A Preliminary Search for Planets and Exozodiacal Emission Around α Centauri A with JWST/MIRI

Aniket Sanghi, Élodie Choquet, Alexis Bidot, William O. Balmer et al.
2 citations
Research Notes of the AAS
Stellar, planetary, and galactic studies
2.31
article

A Preliminary Search for Planets and Exozodiacal Emission Around α Centauri A with JWST/MIRI

Aniket Sanghi, Élodie Choquet, Alexis Bidot, William O. Balmer, N. Godoy, Charles Beichman, Jorge Llop-Sayson, G. Bryden, Billy Quarles, E. Serabyn, Renyu Hu, E. B. Fomalont, Jonathan Aguilar, Michael E. Ressler, Kevin Wagner, Rachel Akeson, Dean C. Hines, Dimitri Mawet, M. C. Wyatt, Maximilian Sommer, P. Kervella, Thomas Henning, Jack J. Lissauer, Jarron Leisenring, Mantas Zilinskas, A. Boccaletti, Marie Ygouf, Laurent Pueyo, Ruslan Belikov, Pierre-Olivier Lagage
article en
2 citations

Abstract

Abstract We present F1550C (15.5 μ m) coronagraphic imaging observations of the nearest solar-type star α Cen A using the James Webb Space Telescope (JWST) Mid-InfraRed Instrument (MIRI). The observations, executed in 2025 February, were compromised by having only one successful roll and degraded performance due to a position mismatch (Δ r ∼ 10 mas) between α Cen A and the best-matching reference observation behind the MIRI coronagraph. We set preliminary upper limits on both the presence of a planet and an exozodiacal dust disk. The observations are sensitive to a planet heated by α Cen A (200–250 K) with a radius ≳1 R Jup at a separation of 1 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>.</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>″</mml:mi> </mml:mrow> </mml:mover> </mml:math> 5 (2 au) and zodiacal dust emission at the level of ≳5–10 times the brightness of our own zodiacal cloud. A complete analysis of all JWST/MIRI observations of α Cen A is forthcoming in Paper I (Beichman &amp; Sanghi et al. 2025, in preparation) and Paper II (Sanghi &amp; Beichman et al. 2025, in preparation).

Research Notes of the AASVol. 9(5)
Openalex Percentile: Top 12%
Stellar, planetary, and galactic studies
2.31
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.