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Mitigation of LEO Satellite Brightness and Trail Effects on the Rubin Observatory LSST (2006.12417v3)

Published 22 Jun 2020 in astro-ph.IM

Abstract: We report studies on the mitigation of optical effects of bright low-Earth-orbit (LEO) satellites on Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST). These include options for pointing the telescope to avoid satellites, laboratory investigations of bright trails on the Rubin Observatory LSST camera sensors, algorithms for correcting image artifacts caused by bright trails, experiments on darkening SpaceX Starlink satellites, and ground-based follow-up observations. The original Starlink v0.9 satellites are g ~ 4.5 mag, and the initial experiment "DarkSat" is g ~ 6.1 mag. Future Starlink darkening plans may reach g ~ 7 mag, a brightness level that enables nonlinear image artifact correction to well below background noise. However, the satellite trails will still exist at a signal-to-noise ratio ~ 100, generating systematic errors that may impact data analysis and limit some science. For the Rubin Observatory 8.4-m mirror and a satellite at 550 km, the full width at half maximum of the trail is about 3" as the result of an out-of-focus effect, which helps avoid saturation by decreasing the peak surface brightness of the trail. For 48,000 LEOsats of apparent magnitude 4.5, about 1% of pixels in LSST nautical twilight images would need to be masked.

Citations (61)

Summary

  • The paper presents methodologies including scheduling algorithms and lab simulations to address satellite trail effects on LSST observations.
  • It validates CCD correction techniques and real-world data analysis to suppress bright trails with minimal observation loss.
  • Collaboration with SpaceX, as shown in the DarkSat initiative, reduces satellite brightness by about 1 magnitude, improving observation quality.

Analysis of Mitigation Strategies for LEO Satellite Impact on Rubin Observatory's LSST

The paper "Mitigation of LEO Satellite Brightness and Trail Effects on the Rubin Observatory LSST" by Tyson et al. investigates the impact of low-Earth-orbit (LEO) satellites, particularly SpaceX's Starlink constellation, on astronomical observations. The paper focuses on the Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST), a project of paramount importance for optical astronomy. The core of the research departs from concerns over the influx of satellite constellations which, if left unchecked, pose a potential threat to ground-based observations by introducing unwanted light artifacts and trails.

Core Investigations and Techniques

  1. Telescope Scheduling and Satellite Avoidance: The paper examines the feasibility of adjusting LSST scheduling algorithms to avoid capturing LEO satellite trails. Simulations demonstrate that avoiding satellites might reduce the number of possible observations, highlighting the difficulty of effectively dodging satellite trails given the LSST's wide field of view.
  2. Laboratory Simulations and Algorithmic Corrections: Laboratory setups replicate satellite trails to examine their impact on LSSTCam charge-coupled devices (CCDs) and explore crosstalk corrections. The research provides initial evidence that nonlinear crosstalk corrections can be developed, enabling the suppression of trail artifacts in the data without significant loss of usable pixels.
  3. Satellite Brightness Reduction Initiatives: The paper details collaboration efforts, particularly with SpaceX, marking a significant attempt at direct mitigation through physical changes in satellite design. The launch and observation of "DarkSat," a Starlink satellite modified to be less reflective, shows a reduction in brightness by approximately 1 mag compared to its progenitors. However, even these mitigated satellites are still above the ideal brightness thresholds for Rubin Observatory.
  4. Real-World Observations and Data Analysis: Observations conducted with the Blanco 4 m telescope using DECam assessed the brightness and trail characteristics of these satellites. The data confirm the effectiveness of the darkening measures and provide a basis for correlating expected with observable trail brightness.

Theoretical Implications and Practical Considerations

The paper illuminates the theoretical challenge of balancing trail mitigation and observational integrity while raising practical considerations for joint space and ground-based efforts. By examining the interoperability of astronomical survey operations with ongoing satellite deployments, this research underscores the necessity for continuous collaborations between scientific and industrial sectors.

Future Developments and Speculative Outcomes

Long-term, the research anticipates further investigations into robust mitigation strategies that include the adoption of improved materials for satellite components, operational avoidance maneuvers, and possibly real-time coordination mechanisms for global observatories. The findings herein are instrumental for ongoing and future LSST-like initiatives across the optical spectrum.

In conclusion, while addressing the nascent yet growing challenge of LEO satellites on astronomical observations, this research provides a template for action in mitigating similar influences on optical astronomy. The paper exemplifies interdisciplinary cooperation in scientific inquiry, hinting at a future where proactive engagement and technological adaptation are continuous priorities in the evolving landscape of sky monitoring.

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