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Betelgeuse scope: Single-mode-fibers-assisted optical interferometer design for dedicated stellar activity monitoring

机译:Betelgeuse范围:单模光纤辅助光学干涉仪设计专用恒星活动监控

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Betelgeuse has gone through a sudden shift in its brightness and dimmed mysteriously. This is likely caused by a hot blob of plasma ejected from Betelgeuse and then cooled to obscuring dust. If true, it is a remarkable opportunity to directly witness the formation of dust around a red supergiant star. Today's optical telescope facilities are not optimized for time-evolution monitoring of the Betelgeuse surface, so in this work, we propose a low-cost optical interferometer. The facility will consist of 12 × 4 inch optical telescopes mounted on the surface of a large radio dish for interferometric imaging; polarization-maintaining single-mode fibers will carry the coherent beams from the individual optical telescopes to an all-in-one beam combiner. A fast steering mirror assisted fiber injection system guides the flux into fibers. A metrology system senses vibration-induced piston errors in optical fibers, and these errors are corrected using fast-steering delay lines. We will present the design.
机译:Betelgeuse已经在其亮度突然转变,神秘地暗淡。这可能是由从Betelgeuse喷射的等离子体热斑,然后冷却至模糊灰尘。如果是的,那么直接见证红色超级星星周围的灰尘是一个显着的机会。今天的光学望远镜设施没有优化对贝格尔格的时间进化监测,所以在这项工作中,我们提出了一种低成本的光学干涉仪。该设施将包括12×4英寸的光学望远镜,安装在用于干涉成分的大型无线电盘的表面上;保持偏振的单模纤维将从各个光学望远镜携带与一体式光束组合器的相干梁。快速转向镜辅助光纤注射系统将通量引导到纤维中。计量系统在光纤中感测振动引起的活塞误差,并且使用快速转向延迟线校正这些误差。我们将展示设计。

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