The Observation of Earth-Like Exoplanets With Ground-Based Telescopes and a Shared Orbiting Starshade

This paper provides the predicted performance of a hybrid space-ground approach that combines a large ground-based telescope such as the Extremely Large Telescope (ELT), the Thirty Meter Telescope (TMT), or the Giant Magellan Telescope (GMT), with a shared orbiting starshade in space. This integration aims to image Earth-like exoplanets around Sun-like stars with deep contrast imaging and an unmatched angular resolution. The starshade forms a deep shadow above the Earth’s atmosphere. However, the presence of atmospheric turbulence requires compensation with adaptive optics to sharpen the images to the diffraction limit. In this paper, we present the expected image plane contrast of the three large telescopes operating with a shared orbiting 99 m diameter starshade, with a detailed analysis focusing on the ELT to measure the reflected light spectra of a solar system, from Venus to Saturn, orbiting a sun-like star. Our analysis utilizes a comprehensive and realistic model of the entire system, incorporating the latest ELT Adaptive Optics (AO) models to mitigate the effects of Earth’s atmospheric turbulence under moderate weather conditions. Our studies show that the ELT AO effectively corrects for these effects, demonstrating minimal impact on sensitivity with different Strehl Ratios (SR) and throughout the full 300–1000 nm bandpass. This includes a comparison with current and future ground- and space-based observatories. We simulate the reflected light images and spectra through Earths atmosphere. We show observation of the major molecular signatures for life, such as oxygen and water on an exo-Earth, leading to a promising avenue for future hybrid space–ground observatories to revolutionize the search for Earth-like planets. Near-term advancements for the implementation of this concept toward deployment will be discussed.