The Royal Road: Eclipsing Binaries and Transiting Exoplanets, 2nd Edition

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Planetary Sciences".

Deadline for manuscript submissions: 24 July 2026 | Viewed by 1736

Special Issue Editors


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Guest Editor
Baja Astronomical Observatory of University of Szeged, Szegedi út, Kt. 766, H-6500 Baja, Hungary
Interests: binary and multiple systems; eclipsing binaries; celestial mechanics
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Guest Editor
Deutsches Zentrum für Luft- und Raumfahrt, Institute of Planetary Research, Rutherfordtstrasse 2, D-12489 Berlin, Germany
Interests: exoplanets; brown dwarfs; Love numbers; exoplanet atmospheres
Special Issues, Collections and Topics in MDPI journals

Special Issue Information

Dear Colleagues,

Two years ago, Universe published a Special Issue devoted to papers on recent results based on ultraprecise photometry obtained using space-telescopes searching for planetary transits. That Special Issue was about eclipsing binary and multiple stars, as well as transiting exoplanets. While the primary goal of these space missions (CoRoT, Kepler, K2, and TESS) was to detect and characterize transiting exoplanets, they also provided thousands of high-duty-cycle and almost-uninterrupted ultraprecise light curves of eclipsing binary stars. They revolutionized the field of exoplanet research and binary star studies. The nine papers published in the former Special Issue, entitled ‘The Royal Road: Eclipsing Binaries and Transiting Exoplanets’, covered wide ranges of the related fields, such as the following:

  • Analyses of tight, multiple-eclipsing triple and quadruple stellar systems;
  • Detections of higher-order gravitational perturbations, and other gravity-induced phenomena in such multiples;
  • Exotic phenomena, e.g., tidal decay in specific exoplanets;
  • Exomoon candidates;
  • Dynamics of circumplanetary disks.

The first Special Issue been touched only the thin surface of the vast and deep ocean that is the science of eclipsing stellar and transiting exoplanetary systems. Therefore, we intend to address these same research areas in a second Special Issue. There is another reason to announce a second Special Issue, namely that, in the meantime, significant progress has been made in these fields due to the continuous operations of such space telescopes like the Transiting Exoplanetary Survey Satellite (TESS) and CHEOPS or, the recently retired instrument, Gaia, which were not covered in the previous Special Issue.

We are looking forward to the PLATO (to be launched in December, 2026), which will provide a vast new ultraprecise photometric database of about 1 million stars. We are also wondering what JWST can do for eclipsing binary and exoplanet research.

Therefore, this second Special Issue will target the same topics, being those related to the analysis and information content of light curves showing eclipsing and transiting events. Some of them are classical problems which are put in a new light in the era of ultraprecise space photometry. Some other issues have become widely observable with space photometry (e.g., only few heart-beat binaries were known by ground-based observations, and hundreds were discovered using space photometry; the beaming effect was found using space photometry using CoRoT for the first time). Instead of giving such a detailed, lengthy list of those effects, we instead call for contributions—original research and review papers—to this Special Issue, which may include any topic related to the extraction of information from eclipse/transit light curves, ETVs/TTVs, the phase curves of eclipsing binary stars, and transiting exoplanets. We encourage submissions on light curve analysis of ultraprecise high-duty-cycle space-based photometries, but contributions are not limited to space-photometry.

We would like to emphasize that this second Special Issue is not limited to the aforementioned areas, but it is open to every aspect of eclipsing binary and transiting exoplanet research that utilizes the photometric time series of these systems. We add that studies of out-of-eclipse/out-of-transit variations, like exoplanetary phase curves, the albedo and other properties of eclipsing binary stars, and statistical analyses of any properties of these systems, their formation, and their evolution are also welcome.

We look forward receiving and publishing the most recent interesting results (and their reviews as well) obtained from the very recent space- and ground-based observations, as well as studies on their theory, in this Special Issue on ‘The Royal Road: Eclipsing Binaries and Transiting Exoplanets, 2nd Edition’ of the journal Universe.

Dr. Tamás Borkovits
Dr. Szilard Csizmadia
Guest Editors

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Keywords

  • eclipsing binaries
  • transiting exoplanets
  • eclipse and transit timing variations
  • hierarchical multiple systems
  • multi-planet systems
  • ellipsoidal, reflection, and beaming effects of binary stars
  • phase curves of exoplanets
  • atmospheres of exoplanets
  • dynamics of multiple systems
  • formation and evolution of binary systems and planetary systems
  • interior structure of stars and planets
  • occurrence rates and frequencies of planets, brown dwarfs, and stars

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Related Special Issue

Published Papers (2 papers)

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Research

36 pages, 11979 KB  
Article
A Few Years Later: Revisiting Period Variations of Eclipsing Binaries in the Northern Continuous Viewing Zone of TESS
by Tamás Borkovits, Tibor Mitnyan, Donát R. Czavalinga and Saul A. Rappaport
Universe 2026, 12(4), 107; https://doi.org/10.3390/universe12040107 - 3 Apr 2026
Viewed by 454
Abstract
In our previous analysis of the eclipse timing variation patterns of eclipsing binaries located in and near the Northern Continuous Viewing Zone (NCVZ) of the TESS space telescope, 135 hierarchical triple star candidates were found. Now, two additional years of TESS observations are [...] Read more.
In our previous analysis of the eclipse timing variation patterns of eclipsing binaries located in and near the Northern Continuous Viewing Zone (NCVZ) of the TESS space telescope, 135 hierarchical triple star candidates were found. Now, two additional years of TESS observations are available and, hence, we have extended the former analysis with the use of the new observational data. We now detect 168 triple star candidates in the updated and reanalyzed sample. The majority (∼74%) of them are identical to the former triples candidates. For many of them, our new solutions are more certain than the original ones. Therefore, we can now conclude that we have identified at least 66 short-period hierarchical triple stellar systems in the NCVZ with full confidence. In the case of the majority of the remaining systems in our sample, the presence of a close third stellar component appears to be very likely. We also identify additional, longer timescale period variations in 34 systems (20% of the total sample) and conclude that in at least three systems the presence of a fourth stellar component is quite plausible. Finally, we report the complete disappearance of the eclipses in two former EBs and detect eclipse depth variations in seven other EBs as well. We interpret this effect as the consequence of changing orbital inclination caused by a non-coplanar third body. Full article
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24 pages, 5297 KB  
Article
TEPCat: The Transiting Extrasolar Planet Catalogue
by John Southworth
Universe 2026, 12(3), 62; https://doi.org/10.3390/universe12030062 - 25 Feb 2026
Viewed by 699
Abstract
Transiting extrasolar planets are extraordinarily valuable for understanding the characteristics and formation of planets, because they are the only exoplanets whose physical and orbital properties can be measured to high precision. Thousands are now known, and it is important to maintain a database [...] Read more.
Transiting extrasolar planets are extraordinarily valuable for understanding the characteristics and formation of planets, because they are the only exoplanets whose physical and orbital properties can be measured to high precision. Thousands are now known, and it is important to maintain a database of them for use by the scientific community. TEPCat performs this task: it is a critical compilation of the physical and observable properties of the known transiting planetary systems. This work introduces the motivation for TEPCat, its scope, contents, and implementation. Example plots of interesting quantities are constructed. The classification of planets and of the eclipse features in their light curves is discussed. TEPCat is maintained and freely available online. Full article
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