On-axis afocal telescopes as framework for Cubesat based astronomical imagers and slit-less spectrographs

TL;DR

This paper proposes afocal telescope designs for Cubesat-based astronomical instruments, aiming to simplify optical systems, enhance throughput, and enable stable fine pointing with off-the-shelf components, suitable for imagers and spectrographs.

Contribution

It introduces afocal telescope frameworks tailored for Cubesats, improving optical simplicity, stability, and reducing development complexity for astronomical imaging and spectroscopy.

Findings

Designs improve throughput and sensitivity over conventional telescopes.

Enable stable fine beam steering using simple tip-tilt mirrors.

Discuss practical implementation aspects like guiding and vibration analysis.

Abstract

Cubesats present unique opportunities for observational astronomy in the modern era. They are useful in observing difficult-to-access wavelength regions and long-term monitoring of interesting astronomical sources. However, conventional telescope designs are not necessarily the best fit for restricted envelope of a Cubesat. Additionally, fine-pointing stability on these platforms is difficult due to the low mass of the spacecraft and special allocations within the optical design are needed to achieve stable pointing. We propose afocal telescope designs as the framework to realise imagers and low-resolution spectrographs on Cubesat platforms. These designs help reduce the number of components in the optical chain and aim to improve throughput and sensitivity compared to conventional designs. Additionally, they also provide a fine steering mechanism within a collimated beam section. Fine beam steering within the collimated beam section avoids issues of image degradation due to out-of-plane rotation of the image plane or offset in the rotation axis of the mirror. This permits the use of simple and mostly off-the-shelf tip-tilt mirrors for beam steering. The designs discussed here also allow for a standard telescope design to be used in many instrument types; thus reducing the complexity as well as the development time and cost. The optical design, performance and SNR estimations of these designs along with some interesting science cases are discussed. A number of practical aspects in implementation such as guiding, tolerancing, choice of detectors, vibration analysis and laboratory test setups are also presented.