Special Issue "Detection and Characterization of Extrasolar Planets"
A special issue of Geosciences (ISSN 2076-3263).
Deadline for manuscript submissions: 30 June 2018
Prof. Dr. Jesus Martinez-Frias
Instituto de Geociencias, IGEO (CSIC-UCM), C/ Del Doctor Severo Ochoa 7, Facultad de Medicina (Edificio Entrepabellones 7 y 8), 28040 Madrid, Spain
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Phone: +34 91 3944829
Fax: +34 91 3944798
Interests: planetary geology; astrobiology; natural resources of near earth space and sustainability; geo and biomarkers; extreme environments and planetary habitability; geodiversity and biodiversity; natural hazards and planetary ecosystems; mineralogy; geoethics in earth and space sciences; geoeducation; science and technology for development; emerging sciences, cultural implications; new paradigms
This Special Issue of Geosciences is dedicated to Exoplantary Science. Exoplanetary science is a vigorous and exciting new area of astrophysics and planetary sciences. Since the revolutionary discovery of a planet orbiting a solar-like star 51 Peg (Mayor and Queloz 1995) about 3600 exoplanets have been discovered in around 2700 planetary systems, which place our unique Solar System into context through the new field of comparative planetology. The radial velocity technique, which is based on detecting changes in the color of a star due to wobble of the host star in response to an exoplanet's gravity, and the photometric transit technique, which is based on measuring the dim in stellar light due to transits of an exoplanet in front of its disk, are the two main techniques that have been used to detect and characterize most known exoplanets. Other techniques, namely, gravitational microlensing, astrometry, and direct imaging, also have been used to detect several exoplanets. Recent and upcoming ground and space-based telescopes and facilities, which provide high-precision photometric and spectroscopic observations, allow us to accurately detect and characterize exoplanetary systems, including their atmosphere and architectures. Thus, we are living in an exciting time, in which we have been detecting Earth-sized exoplanets in the habitable zone of their host stars, and we are getting closer to the detection of Earth twins. The comprehensive information about exoplanetary systems and their host stars combined with our knowledge of solar system’s content will lead us toward a complete understanding about the exoplanetary atmospheres, their potential geodynamics, formation, evolution, and habitability conditions.
Therefore, the main goal of this Special Issue of Geosciences is to collect papers on original research, inspiring reviews, and an outlook of open and challenging problems in the near future.
It is recommended that authors approach the Guest Editor at an early stage about possible submissions in order to verify the appropriateness of their potential contributions. If appropriate, an abstract will be requested, and the corresponding author will be required to submit the full manuscript online by the deadline of 30 June 2018.
Dr. Mahmoudreza Oshagh
Prof. Dr. Jesus Martinez-Frias
Manuscript Submission Information
Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All papers will be peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.
Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Geosciences is an international peer-reviewed open access quarterly journal published by MDPI.
Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 350 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.
- exoplanet detection
- exoplanet characterization
- stellar activity induced noise
- future instrumentation
- exoplanets’ atmosphere
- architecture of exoplanet systems
The below list represents only planned manuscripts. Some of these manuscripts have not been received by the Editorial Office yet. Papers submitted to MDPI journals are subject to peer-review.
Preliminary topic: The Role of Stellar Chemistry on the Formation of Exoplanets
Corresponding Author: Dr. Vardan Adibekyan (Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal)
Preliminary topic: The Detection of Earth-mass Planets amid Stellar-induced Noise
Corresponding Author: Dr. João Faria (Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal)
Preliminary topic: Microlensing Searches for Exoplanets
Corresponding Author: Dr. Yiannis Tsapras (Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr 12-14, D-69120 Heidelberg, Germany)
Preliminary topic: Direct Imaging and Characterization of Free-floating Planetary-mass Objects
Corresponding Author: Dr. José A. Caballero (Landessternwarte Königstuhl, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany / Centro de Astrobiología (CSIC-INTA), ESAC Campus, Madrid, Spain)