Elisabeth C. Matthews on Muck Rack

Elisabeth C. Matthews

As seen in: Nature
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Author Correction: A super-massive Neptune-sized planet - Nature

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By Luca Naponiello, Tiziano Zingales, Luigi Mancini, Alessandro Sozzetti, Aldo S. Bonomo, Li Zeng, Zoe M. Leinhardt, Katia Biazzo, Matteo Pinamonti, Daniele Locci, Antonio Maggio, Antonino F. Lanza, Jack J. Lissauer, Philip Carter, Andrea Bignamini, Walter Boschin, Luke Bouma, Xavier Dumusque, Akihiko Fukui, Paolo Giacobbe, Adriano Ghedina, Gloria Guilluy, Aaron Thomas , John F. Kielkopf, Luca Malavolta, Andrew Mann, Rachel Matson, Elisabeth C. Matthews, Domenico Nardiello, Norio Narita, Emanuele Pace, Isabella Pagano, Enric Pallé, Sara Seager, Avi Shporer, Joseph D. Twicken, Joshua Winn
| Nature
Open in Who Shared Issue with article?

A super-massive Neptune-sized planet - Nature

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By Luigi Mancini, Li Zeng, Katia Biazzo, Antonio Maggio, Jack J. Lissauer, Philip Carter, Luke Bouma, Akihiko Fukui, Paolo Giacobbe, Aaron Thomas , John F. Kielkopf, Andrew Mann, Rachel Matson, Norio Narita, Isabella Pagano, Enric Pallé, Sara Seager, Avi Shporer, Joseph D. Twicken, Joshua Winn, Luca Naponiello, Alessandro Sozzetti, Aldo S. Bonomo, Zoe M. Leinhardt, Matteo Pinamonti, Daniele Locci, Antonino F. Lanza, Andrea Bignamini, Walter Boschin, Xavier Dumusque, Adriano Ghedina, Gloria Guilluy, Luca Malavolta, Elisabeth C. Matthews, Domenico Nardiello, Emanuele Pace
| Nature
Abstract Neptune-sized planets exhibit a wide range of compositions and densities, depending on factors related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relatively low-density planets with thick hydrogen–helium atmospheres1,2 to higher-density planets with a substantial amount of water or a rocky interior with a thinner atmosphere, such as HD 95338 b (ref. 3), TOI-849 b (ref. 4) and TOI-2196 b (ref. 5).
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