The Polstar High Resolution Spectropolarimetry MIDEX Mission

Abstract

The Polstar mission will provide for a space-borne 60cm telescope operating at UV wavelengths with spectropolarimetric capability capturing all four Stokes parameters (intensity, two linear polarization components, and circular polarization). Polstar's capabilities are designed to meet its goal of determining how circumstellar gas flows alter massive stars' evolution, and finding the consequences for the stellar remnant population and the stirring and enrichment of the interstellar medium, by addressing four key science objectives. In addition, Polstar will determine drivers for the alignment of the smallest interstellar grains, and probe the dust, magnetic fields, and environments in the hot diffuse interstellar medium, including for the first time a direct measurement of the polarized and energized properties of intergalactic dust. Polstar will also characterize processes that lead to the assembly of exoplanetary systems and that affect exoplanetary atmospheres and habitability. Science driven design requirements include: access to ultraviolet bands: where hot massive stars are brightest and circumstellar opacity is highest; high spectral resolution: accessing diagnostics of circumstellar gas flows and stellar composition in the far-UV at 122-200nm, including the NV, SiIV, and CIV resonance doublets and other transitions such as NIV, AlIII, HeII, and CIII; polarimetry: accessing diagnostics of circumstellar magnetic field shape and strength when combined with high FUV spectral resolution and diagnostics of stellar rotation and distribution of circumstellar gas when combined with low near-UV spectral resolution; sufficient signal-to-noise ratios: ~1000 for spectropolarimetric precisions of 0.1% per exposure; ~100 for detailed spectroscopic studies; ~10 for exploring dimmer sources; and cadence: ranging from 1-10 minutes for most wind variability studies.

13 pages, 6 figures, presented at SPIE Optics and Photonics 2021

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• Polarization Variability Arising from Clumps in the Winds of Wolf-Rayet Stars
• A compact gaseous accretion disk in Keplerian rotation around MWC147
• Ultraviolet Spectropolarimetry with Polstar: Interstellar Medium Science
• Magnetospheric Accretion in Classical T Tauri Stars
• Ultraviolet Spectropolarimetry:Conservative and Nonconservative Mass Transfer in OB Interacting Binaries
• UV Spectropolarimetry with Polstar: Massive Star Binary Colliding Winds
• Ultraviolet Spectropolarimetry With Polstar: Using Polstar to test Magnetospheric Mass-loss Quenching
• Ultraviolet Spectropolarimetry: Investigating stellar magnetic field diagnostics
• UV Spectropolarimetry with Polstar: Protoplanetary Disks
• Ultraviolet Spectropolarimetry with Polstar: Clumping and Mass-loss Rate Corrections
• The UVMag space project: UV and visible spectropolarimetry of massive stars

Cited by in corpus (10)

• Exoplanet weather and climate regimes with clouds and thermal ionospheres: A model grid study in support of large-scale observational campaigns
• Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars
• Ultraviolet Spectropolarimetry:Conservative and Nonconservative Mass Transfer in OB Interacting Binaries
• Ultraviolet Spectropolarimetry with Polstar: Interstellar Medium Science
• UV Spectropolarimetry with Polstar: Massive Star Binary Colliding Winds
• Ultraviolet Spectropolarimetric Diagnostics of Hot Star Magnetospheres
• Ultraviolet Spectropolarimetry: Investigating stellar magnetic field diagnostics
• Ultraviolet Spectropolarimetry With Polstar: Using Polstar to test Magnetospheric Mass-loss Quenching
• UV Spectropolarimetry with Polstar: Protoplanetary Disks
• Ultraviolet Spectropolarimetry with Polstar: Clumping and Mass-loss Rate Corrections