TESS light curve and apsidal motion in the eccentric eclipsing binary V871 Aquilae

Key Points

• Apsidal motion data highlights the complexity of orbital parameters for V871 Aquilae, enhancing our understanding of binary systems.
• Key metrics show significant variations in the light curve, suggesting unique features in the eclipse behavior of the system.
• Analysis conducted on the light curve data from TESS to assess the orbital characteristics of the eclipsing binary star.
• Findings imply further exploration of eccentric binary systems may provide insights into stellar evolution.