Analysis of physical properties of the HAT-P-12b planetary system
Main Article Content
Abstract
The exoplanet HAT-P-12b was observed at the Sierra Remote Observatories by a 0.7 meters diameter reflective robotic telescope CDK700 with the CCD photometric technique. This research using 317 images of the HAT-P-12b on April 14, 2017. They were analyzed the photometric photometry and calculated the physical properties by the AstroImageJ program. The results show that the radius of the exoplanet HAT-P-12b is 0.951 RJ, orbital period P about 3.2105 days. The center of page traverse Tc is 2457857.166110000 (BJD) and the total time of traverse T is 0.093519 days. The Star and Exoplanet View program was created the HAT-P-12b model that the decreasing brightness with 1.94864 percent the average distance between the exoplanet HAT-P-12b and the center is 0.0388 AU.
Downloads
Metrics
Article Details
Licensing
TURCOMAT publishes articles under the Creative Commons Attribution 4.0 International License (CC BY 4.0). This licensing allows for any use of the work, provided the original author(s) and source are credited, thereby facilitating the free exchange and use of research for the advancement of knowledge.
Detailed Licensing Terms
Attribution (BY): Users must give appropriate credit, provide a link to the license, and indicate if changes were made. Users may do so in any reasonable manner, but not in any way that suggests the licensor endorses them or their use.
No Additional Restrictions: Users may not apply legal terms or technological measures that legally restrict others from doing anything the license permits.