Astrometric detection of exoplanets

Fuente: arXiv
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Autore principale: Feng, Fabo
Natura: Preprint
Pubblicazione: 2024
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author Feng, Fabo
author_facet Feng, Fabo
contents As the most ancient branch of astronomy, astrometry has been developed for thousands of years. However, it has only recently become possible to utilize astrometry for the detection of exoplanets. Gaia, an astrometric surveyor of 1 billion stars, is capable of measuring the position of stars with a precision as high as 20 $μ$as. Gaia is expected to discover more than 10,000 exoplanets by the end of its mission, surpassing the productivity of most exoplanet surveys. In this chapter, I will introduce different techniques used to achieve high-precision astrometry. Subsequently, I will explore how both relative and absolute astrometry can be employed to detect exoplanets. Finally, I will present the detection limit of the Gaia astrometric survey.
format Preprint
id arxiv_https___arxiv_org_abs_2403_08226
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Astrometric detection of exoplanets
Feng, Fabo
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
As the most ancient branch of astronomy, astrometry has been developed for thousands of years. However, it has only recently become possible to utilize astrometry for the detection of exoplanets. Gaia, an astrometric surveyor of 1 billion stars, is capable of measuring the position of stars with a precision as high as 20 $μ$as. Gaia is expected to discover more than 10,000 exoplanets by the end of its mission, surpassing the productivity of most exoplanet surveys. In this chapter, I will introduce different techniques used to achieve high-precision astrometry. Subsequently, I will explore how both relative and absolute astrometry can be employed to detect exoplanets. Finally, I will present the detection limit of the Gaia astrometric survey.
title Astrometric detection of exoplanets
topic Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2403.08226