# Upper limits on the water vapour content of the $\beta$ Pictoris debris   disk

**Authors:** M. Cavallius, G. Cataldi, A. Brandeker, G. Olofsson, B. Larsson, R., Liseau

arXiv: 1906.11106 · 2019-08-21

## TL;DR

This study sets upper limits on water vapor in the $eta$ Pictoris debris disk by analyzing Herschel data, suggesting the gas composition is similar to that of some solar system comets.

## Contribution

First upper limits on H$_2$O gas mass in the $eta$ Pictoris disk using archival Herschel data and radiative transfer modeling.

## Key findings

- H$_2$O line undetected in Herschel data
- Upper limit on H$_2$O mass between 7.4×10^{16} and 1.1×10^{18} kg
- Gas-phase CO/H$_2$O ratios marginally consistent with low-ratio solar system comets

## Abstract

The debris disk surrounding $\beta$~Pictoris has been observed with ALMA to contain a belt of CO gas with a distinct peak at $\sim$85 au. This CO clump is thought to be the result of a region of enhanced density of solids that collide and release CO through vaporisation. The parent bodies are thought to be comparable to solar system comets, in which CO is trapped inside a water ice matrix. Since H$_2$O should be released along with CO, we aim to put an upper limit on the H$_2$O gas mass in the disk of $\beta$ Pictoris. We use archival data from the Heterodyne Instrument for the Far-Infrared (HIFI) aboard the Herschel Space Observatory to study the ortho-H$_2$O 1$_{10}$-1$_{01}$ emission line. The line is undetected. Using a python implementation of the radiative transfer code RADEX, we convert upper limits on the line flux to H$_2$O gas masses. The resulting lower limits on the CO/H$_2$O mass ratio are compared to the composition of solar system comets. Depending on the assumed gas spatial distribution, we find a 95% upper limit on the ortho-H$_2$O line flux of $7.5 \times 10^{-20}$ W m$^{-2}$ or $1.2 \times 10^{-19}$ W m$^{-2}$. These translate into an upper limit on the H$_2$O mass of $7.4 \times 10^{16}$-$1.1 \times 10^{18}$ kg depending on both the electron density and gas kinetic temperature. The range of derived gas-phase CO/H$_2$O ratios is marginally consistent with low-ratio solar system comets.

## Full text

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## Figures

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## References

43 references — full list in the complete paper: https://tomesphere.com/paper/1906.11106/full.md

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Source: https://tomesphere.com/paper/1906.11106