# TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR   858

**Authors:** Andrew Vanderburg, Chelsea X. Huang, Joseph E. Rodriguez, Juliette C., Becker, George R. Ricker, Roland K. Vanderspek, David W. Latham, Sara Seager,, Joshua N. Winn, Jon M. Jenkins, Brett Addison, Allyson Bieryla, Cesar, Brice\~no, Brendan P. Bowler, Timothy M. Brown, Christopher J. Burke,, Jennifer A. Burt, Douglas A. Caldwell, Jake T. Clark, Ian Crossfield, Jason, A. Dittmann, Scott Dynes, Benjamin J. Fulton, Natalia Guerrero, Daniel, Harbeck, Jonathan Horner, Stephen R. Kane, John Kielkopf, Adam L. Kraus,, Laura Kreidberg, Nicolas Law, Andrew W. Mann, Matthew W. Mengel, Timothy D., Morton, Jack Okumura, Logan A. Pearce, Peter Plavchan, Samuel N. Quinn,, Markus Rabus, Mark E. Rose, Pam Rowden, Avi Shporer, Robert J. Siverd,, Jeffrey C. Smith, Keivan Stassun, C.G. Tinney, Rob Wittenmyer, Duncan J., Wright, Hui Zhang, George Zhou, and Carl A. Ziegler

arXiv: 1905.05193 · 2019-08-14

## TL;DR

TESS discovered a compact system of three super-Earths around the nearby star HR 858, with potential for detailed follow-up studies due to their favorable observational properties.

## Contribution

This study presents the first detailed characterization of a multi-planet system around HR 858, utilizing novel data analysis techniques and combined space- and ground-based observations.

## Key findings

- Three planets approximately twice Earth's size transiting HR 858.
- Two planets may be in mean motion resonance.
- The system is suitable for future radial velocity and spectroscopic studies.

## Abstract

Transiting Exoplanet Survey Satellite (TESS) observations have revealed a compact multi-planet system around the sixth-magnitude star HR 858 (TIC 178155732, TOI 396), located 32 parsecs away. Three planets, each about twice the size of Earth, transit this slightly-evolved, late F-type star, which is also a member of a visual binary. Two of the planets may be in mean motion resonance. We analyze the TESS observations, using novel methods to model and remove instrumental systematic errors, and combine these data with follow-up observations taken from a suite of ground-based telescopes to characterize the planetary system. The HR 858 planets are enticing targets for precise radial velocity observations, secondary eclipse spectroscopy, and measurements of the Rossiter-McLaughlin effect.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1905.05193/full.md

## References

80 references — full list in the complete paper: https://tomesphere.com/paper/1905.05193/full.md

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Source: https://tomesphere.com/paper/1905.05193