Detection and Characterization of Extrasolar Planets
A special issue of Geosciences (ISSN 2076-3263).
Deadline for manuscript submissions: closed (30 June 2018) | Viewed by 40922
Interests: extrasolar planets; stellar magnetic activity; planetary atmosphere; eclipsing binaries; architecture of exoplanet systems
Interests: planetary geosciences; meteorites; geoeducation; geoethics; mineralogy; geochemistry; sustainability; conceptual changes; astrobiology; future earth
Special Issues, Collections and Topics in MDPI journals
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 submissions that pass pre-check are 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 monthly 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 1800 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