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Updated: May 17, 2026

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
Published on: May 10, 2020
Flight demonstration of a milliarcsecond pointing system for direct exoplanet imaging
Christopher B Mendillo1, Supriya Chakrabarti, Timothy A Cook
1Astronomy Department, Boston University, Boston, Massachusetts 02215, USA. christopher.mendillo@gmail.com
The Planetary Imaging Concept Testbed Using a Rocket Experiment (PICTURE) achieved exceptional pointing stability for exozodiacal dust imaging. Its fine pointing system reached 5.1 mas RMS, comparable to the Hubble Space Telescope.
Area of Science:
- * Astrophysics
- * Optical Engineering
Background:
- * Direct imaging of exozodiacal dust disks is crucial for characterizing exoplanetary systems.
- * Previous rocket-based experiments have faced challenges in achieving the necessary pointing stability for high-contrast imaging.
Purpose of the Study:
- * To present flight results from the optical pointing control system of the PICTURE sounding rocket.
- * To evaluate the performance of the fine pointing system (FPS) in stabilizing the telescope beam for exozodiacal dust imaging.
Main Methods:
- * Utilized a visible nulling coronagraph to attempt direct imaging of the exozodiacal dust disk of ϵ Eridani.
- * Implemented a fine pointing system (FPS) with an angle tracker camera and fast steering mirror.
- * Analyzed the power spectral density of the FPS and rocket attitude control system (ACS) in-flight performance.
Main Results:
- * The rocket's attitude control system (ACS) provided 627 mas RMS body pointing.
- * The PICTURE fine pointing system (FPS) successfully stabilized the telescope beam to 5.1 mas RMS.
- * Achieved pointing stability comparable to the Hubble Space Telescope.
Conclusions:
- * The PICTURE mission demonstrated a highly stable optical pointing control system suitable for exoplanetary science.
- * The achieved pointing precision validates the FPS design for future high-contrast imaging missions.
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