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Der Stern Beta Pictoris ist der zweithellste in der Konstellation Maler am Südhimmel und besitzt zwei bekannte Planeten, Beta Pictoris b und Beta Pictoris c. Letzterer umkreist seinen Mutterstern auf einer derart engen Umlaufbahn, dass ihn selbst die besten Teleskope der Welt bisher nicht direkt abbilden konnten. Nature, 433, 133 paper   arxiv, Ro-vibrational CO Detected in the $\beta$~Pictoris Circumstellar Disk HAHN J. arxiv, Constraints on the occurrence and distribution of 1--20 MJup companions to stars at separations of 5--5000 AU from a compilation of direct imaging surveys A. NOWAK M., LACOUR S., LAGRANGE A.-M., RUBIBI P., WANG J. et al. Astron. Ann. ApJ, 823, 6 2014 et al. Astron. ADS, Light Scattering and Thermal Emission by Primitive Dust Particles in Planetary Systems 2001 ADS, A Model-Independent Mass and Moderate Eccentricity for β Pic b SPIE, 10698, 1069821 2014 The bigger the exoplanet, the bigger the gravitational tug it exerts on the star. 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