4.6 Article

TIC 168789840: A Sextuply Eclipsing Sextuple Star System

期刊

ASTRONOMICAL JOURNAL
卷 161, 期 4, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-3881/abddb5

关键词

Eclipsing binary stars; Transit photometry; Multiple stars; Astronomy data analysis

资金

  1. NASA's Science Mission directorate
  2. NASA [NAS5-26555]
  3. Ministry of Education of the Czech Republic [LM2018102, MSMT-CR LTT18004]
  4. MSMT/EU funds [CZ.02.1.01/0.0/0.0/16_013/0001402]
  5. Hungarian National Research, Development and Innovation Office-NKFIH Grant [KH-130372]
  6. MIT's Kavli Institute

向作者/读者索取更多资源

The sextuple star system TIC 168789840 is composed of three eclipsing binaries arranged in a hierarchical structure. Follow-up observations and speckle interferometry have provided insights into the system's parameters and characteristics. The system's rare composition and structure offer valuable new insights into the formation, dynamics, and evolution of multiple star systems.
We report the discovery of a sextuply eclipsing sextuple star system from TESS data, TIC 168789840, also known as TYC 7037-89-1, the first known sextuple system consisting of three eclipsing binaries. The target was observed in Sectors 4 and 5 during Cycle 1, with lightcurves extracted from TESS Full Frame Image data. It was also previously observed by the WASP survey and ASAS-SN. The system consists of three gravitationally bound eclipsing binaries in a hierarchical structure of an inner quadruple system with an outer binary subsystem. Follow-up observations from several different observatories were conducted as a means of determining additional parameters. The system was resolved by speckle interferometry with a 042 separation between the inner quadruple and outer binary, inferring an estimated outer period of similar to 2 kyr. It was determined that the fainter of the two resolved components is an 8.217 day eclipsing binary, which orbits the inner quadruple that contains two eclipsing binaries with periods of 1.570 days and 1.306 days. Markov Chain Monte Carlo (MCMC) analysis of the stellar parameters has shown that the three binaries of TIC 168789840 are triplets, as each binary is quite similar to the others in terms of mass, radius, and T-eff. As a consequence of its rare composition, structure, and orientation, this object can provide important new insight into the formation, dynamics, and evolution of multiple star systems. Future observations could reveal if the intermediate and outer orbital planes are all aligned with the planes of the three inner eclipsing binaries.

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