Mauve: a UV-Vis satellite dedicated to monitor stellar activity and variability

中国科学院云南天文台学术报告通知

2025年第31

报告题目Mauve: a UV-Vis satellite dedicated to monitor stellar activity and variability

报告人Parul Janagal

报告人单位Blue Skies Space

报告语言English

报告时间2025717日(星期四)10:00-11:00

报告地点科研1号楼412会议室

报告摘要

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Mauve is a small satellite equipped with a 13-cm telescope and a UV-Visible spectrophotometer (with an operative wavelength range of 200-700 nm) conceived to measure the stellar magnetic activity and variability. It is scheduled for launch in October 2025 and is currently under construction. The Mauve science program will be delivered via a multi-year collaborative survey program, with thousands of hours each year available for long baseline observations of hundreds of stars, unlocking a significant time domain astronomy opportunity. Mauve’s mission lifetime is 3 years with the ambition of 5 years, and will cover a broad field of regard (–46.4 to 31.8 degrees in ICRS) during this period.

This facility was conceived to support pilot studies and new ideas in science and is fully dedicated to time-domain astronomy. The main surveys to be executed by Mauve are long baseline observations of flare stars, Herbig Ae/Be stars, exoplanet hosts, as well as contact binary variables (RS CVn variables, symbiotic stars, Algol-type stars, etc.). Besides these major science themes, the spectrometer data can be utilised to support and complement existing and upcoming facilities as a pathfinder, or conduct simultaneous/follow-up observations.

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报告人简介:

Parul Janagal leads the science outreach efforts at Blue Skies Space. She completed her PhD at the Indian Institute of Technology Indore, where she researched the emission from radio pulsars using uGMRT (upgraded Giant Metrewave Radio Telescope) and MWA (Murchison Widefield Array).


云台邀请方:恒星物理研究团组

邀请方联系人:闫冬冬 




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