Is Beta Pic b the transiting planet of November 1981?
A. Lecavelier des Etangs, A. Vidal-Madjar

TL;DR
This paper investigates whether the directly imaged planet Beta Pic b could be the same object responsible for the 1981 photometric transit event, by analyzing its orbital parameters and historical observations.
Contribution
It provides a detailed analysis linking the 1981 photometric event to the orbit of Beta Pic b, estimating its orbital parameters and predicting future transits.
Findings
Estimated semi-major axis: 7.6-8.7 AU
Orbital period: 15.9-19.5 years
Predicted future transits and imaging opportunities
Abstract
In 1981, Beta Pictoris showed strong and rapid photometric variations that were attributed to the transit of a giant comet or a planet orbiting at several AUs (Lecavelier des Etangs et al. 1994, 1995, 1997; Lamers et al. 1997). Recently, a candidate planet has been identified by imagery in the circumstellar disk of Beta Pictoris (Lagrange et al. 2009). This planet, named Beta Pic b, is observed at a projected distance of 8AU from the central star. It is therefore a plausible candidate for the photometric event observed in 1981. The coincidence of the observed position of the planet in November 2003 and the calculated position assuming that the 1981 transit is due to a planet orbiting at 8 AU is intriguing. Assuming that the planet that is detected on the image is the same as the object transiting in November 1981, we estimate ranges of possible orbital distances and periods. In the…
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