Analysis of an eclipsing binary system
GSC 2496-448
Gemma Còdol Cugat July 7th, 2022 Instituto de Astrofísica de Canarias (IAC) Joves i Ciència program
Eclipsing binaries
A binary system that is aligned with the viewer's plane of sight, producing periodic transits and eclipses
Source: University of California, Santa Barbara
Light curves
GSC 2496-448
GSC 2496-448 light curves
April 13th, 2019
April 25th, 2019
April 27th, 2019
April 26th, 2019
3. 1. Period
T = 0.3001 ± 0.001 days or 7h 10min
Relative magnitude
Phase
3.2. Semimajor axis and total system mass
by means of Kepler's third law:
a ≈ 0,0088 AU
MT ≈ 3,9156 M☉
Thanks!
Analysis of an eclipsing binary system
Gemma Còdol Cugat
Created on July 5, 2022
Start designing with a free template
Discover more than 1500 professional designs like these:
View
Practical Presentation
View
Smart Presentation
View
Essential Presentation
View
Akihabara Presentation
View
Pastel Color Presentation
View
Modern Presentation
View
Relaxing Presentation
Explore all templates
Transcript
Analysis of an eclipsing binary system
GSC 2496-448
Gemma Còdol Cugat July 7th, 2022 Instituto de Astrofísica de Canarias (IAC) Joves i Ciència program
Eclipsing binaries
A binary system that is aligned with the viewer's plane of sight, producing periodic transits and eclipses
Source: University of California, Santa Barbara
Light curves
GSC 2496-448
GSC 2496-448 light curves
April 13th, 2019
April 25th, 2019
April 27th, 2019
April 26th, 2019
3. 1. Period
T = 0.3001 ± 0.001 days or 7h 10min
Relative magnitude
Phase
3.2. Semimajor axis and total system mass
by means of Kepler's third law:
a ≈ 0,0088 AU
MT ≈ 3,9156 M☉
Thanks!