Title

Neutrino and EM asterometric detection of habitable exoplanets

Authors

Paul Shapshak*

Affiliation

¹Global Disease Institute, Tampa General Hospital, Department of Internal Medicine, Morsani College of Medicine, University of South Florida, Tampa, Florida 33606, USA. ^*Corresponding author:

Email

Paul Shapshak – E-mail: pshapshak@gmail.com        

Article Type

Editorial

Date

Received March 1, 2023; Revised March 31, 2023; Accepted March 31, 2023, Published March 31, 2023

Discovering habitable exoplanets and exomoons increases the possibility of detecting extraterrestrial life. A bilateral approach, using neutrino and electromagnetic (EM) radiation technologies, can be used to simultaneously characterize star types that generally have exoplanets and exomoons.  This includes cool main-sequence, sub-giant, and red-giant stars. Additionally, supernovae, black holes, and neutron and dwarf stars, will be included to widen the investigation, since they sometimes have companions, including stars and planets. Currently, space exploration is advancing beyond the solar system and proliferating into deep space. For this expansion, sophisticated artificial intelligence (AI) is required and being developed for self-coordination and interactive regulation of the various exploratory vehicles and telescopes. [1-6]

Keywords

Neutrino and EM asterometric detection of habitable exoplanets

Citation

Shapshak et al. Bioinformation 19(3): 235-237 (2023)

Edited by

P Kangueane

ISSN

0973-2063

Publisher

Biomedical Informatics

License

This is an Open Access article which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited. This is distributed under the terms of the Creative Commons Attribution License.