arXiv · 2207.03293
The GAPS Programme at TNG XL: A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422
Abstract
We investigate the exoplanet candidate TOI-1422b, which was discovered by the TESS space telescope around the high proper-motion G2V star TOI-1422 ($V=10.6$ mag), 155pc away, with the primary goal of confirming its planetary nature and characterising its properties. We monitored TOI-1422 with the HARPS-N spectrograph for 1.5 years to precisely quantify its radial velocity variation. The radial velocity measurements are analyzed jointly with TESS photometry and we also check for blended companions through high-spatial resolution images using the AstraLux instrument. We estimate that the parent star has a radius and a mass of $R^*=1.019_{-0.013}^{+0.014} R_{\odot}$, $M^*=0.981_{-0.065}^{+0.062} M_{\odot}$, respectively. Our analysis confirms the planetary nature of TOI-1422b and also suggests the presence of a Neptune-mass planet on a more distant orbit, the candidate TOI-1422c, which is not detected in TESS light curves. The inner planet, TOI-1422b, orbits on a period $P_{\rm b}=12.9972\pm0.0006$ days and has an equilibrium temperature $T_{\rm eq, b}=867\pm17$ K. With a radius of $R_{\rm b}=3.96^{+0.13}_{-0.11} R_{\oplus}$, a mass of $M_{\rm b}=9.0^{+2.3}_{-2.0} M_{\oplus}$ and, consequently, a density of $\rho_{\rm b}=0.795^{+0.290}_{-0.235}$ g cm$^{-3}$, it can be considered a warm Neptune-size planet. Compared to other exoplanets of similar mass range, TOI-1422b is among the most inflated ones and we expect this planet to have an extensive gaseous envelope that surrounds a core with a mass fraction around $10\%-25\%$ of the total mass of the planet. The outer non-transiting planet candidate, TOI-1422c, has an orbital period of $P_{\rm c}=29.29^{+0.21}_{-0.20}$ days, a minimum mass, $M_{\rm c}\sin{i}$, of $11.1^{+2.6}_{-2.3} M_{\oplus}$, an equilibrium temperature of $T_{\rm eq, c}=661\pm13$ K and, therefore, if confirmed, it could be considered as another warm Neptune.
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L. Naponiello, L. Mancini, M. Damasso, A. S. Bonomo, A. Sozzetti, D. Nardiello, K. Biazzo, R. G. Stognone, J. Lillo-Box, A. F. Lanza, E. Poretti, J. J. Lissauer, L. Zeng, A. Bieryla, G. Hébrard, M. Basilicata, S. Benatti, A. Bignamini, F. Borsa, R. Claudi, R. Cosentino, E. Covino, A. de Gurtubai, X. Delfosse, S. Desidera, D. Dragomir, J. D. Eastman, Z. Essack, A. F. M. Fiorenzano, P. Giacobbe, A. Harutyunyan, N. Heidari, C. Hellier, J. M. Jenkins, C. Knapic, P. -C. König, D. W. Latham, A. Magazzù, A. Maggio, J. Maldonado, G. Micela, E. Molinari, M. Molinaro, E. H. Morgan, C. Moutou, V. Nascimben, E. Pace, I. Pagano, M. Pedani, G. Piotto, M. Pinamonti, E. V. Quintana, M. Rainer, G. R. Ricker, S. Seager, J. D. Twicken, R. Vanderspek, J. N. Winn. 2022-07-07. The GAPS Programme at TNG XL: A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422. https://doi.org/10.1051/0004-6361%2F202244079
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