Potential for Solar System Science with the ngVLA
Abstract
Radio wavelength observations of solar system bodies are a powerful method of probing many characteristics of those bodies. From surface and subsurface, to atmospheres (including deep atmospheres of the giant planets), to rings, to the magnetosphere of Jupiter, these observations provide unique information on the current state, and sometimes history, of the bodies. The ngVLA will enable the highest sensitivity and resolution observations of this kind, with the potential to revolutionize our understanding of some of these bodies. In this article, we present a review of state-of-the-art radio wavelength observations of a variety of bodies in our solar system, varying in size from ring particles and small near-Earth asteroids to the giant planets. Throughout the review we mention improvements for each body (or class of bodies) to be expected with the ngVLA. A simulation of a Neptune-sized object is presented in Section 6. Section 7 provides a brief summary for each type of object, together with the type of measurements needed for all objects throughout the Solar System.
Additional Information
© 2018 Astronomical Society of the Pacific.Attached Files
Accepted Version - 1810.08521.pdf
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Additional details
- Eprint ID
- 94948
- DOI
- 10.48550/arXiv.1810.08521
- Resolver ID
- CaltechAUTHORS:20190424-151716678
- Created
-
2019-04-24Created from EPrint's datestamp field
- Updated
-
2023-06-02Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department
- Series Name
- ASP Conference Series
- Series Volume or Issue Number
- 7