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Record W2512958393 · doi:10.3847/0004-6256/152/6/160

A 1.9 EARTH RADIUS ROCKY PLANET AND THE DISCOVERY OF A NON-TRANSITING PLANET IN THE KEPLER-20 SYSTEM*

2016· article· en· W2512958393 on OpenAlexfundno aff
Lars A. Buchhave, Courtney D. Dressing, X. Dumusque, Ken Rice, Andrew Vanderburg, Annelies Mortier, Mercedes López‐Morales, Eric Lopez, M. Lundkvist, H. Kjeldsen, L. Affer, A. S. Bonomo, David Charbonneau, A. Collier Cameron, R. Cosentino, P. Figueira, A. F. Martínez Fiorenzano, A. Harutyunyan, R. D. Haywood, John Asher Johnson, David W. Latham, C. Lovis, L. Malavolta, M. Mayor, E. Molinari, F. Motalebi, V. Nascimbeni, F. Pepe, David F. Phillips, G. Piotto, D. Pollacco, D. Queloz, Dimitar Sasselov, D. Ségransan, A. Sozzetti, S. Udry, Chris Watson

Bibliographic record

VenueThe Astronomical Journal · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersFundação para a Ciência e a TecnologiaSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryUniversité de GenèveDanmarks GrundforskningsfondScience and Technology Facilities CouncilNational Research FoundationQueen's University BelfastUniversity of St AndrewsScottish Universities Physics AllianceCalifornia Institute of TechnologyEuropean CommissionStellar Astrophysics CentreQueen's UniversityNASA Exoplanet Science InstituteNational Aeronautics and Space AdministrationJohn Templeton FoundationSmithsonian InstitutionDanmarks Frie ForskningsfondNational Science Foundation
KeywordsPhysicsPlanetKeplerAstrobiologyAstronomyEarth radiusRADIUSKepler-69cEarth (classical element)Planetary systemTerrestrial planetAstrophysics

Abstract

fetched live from OpenAlex

ABSTRACT Kepler-20 is a solar-type star ( V = 12.5) hosting a compact system of five transiting planets, all packed within the orbital distance of Mercury in our own solar system. A transition from rocky to gaseous planets with a planetary transition radius of ∼1.6 has recently been proposed by several articles in the literature. Kepler-20b ( ∼ 1.9 ) has a size beyond this transition radius; however, previous mass measurements were not sufficiently precise to allow definite conclusions to be drawn regarding its composition. We present new mass measurements of three of the planets in the Kepler-20 system that are facilitated by 104 radial velocity measurements from the HARPS-N spectrograph and 30 archival Keck/HIRES observations, as well as an updated photometric analysis of the Kepler data and an asteroseismic analysis of the host star ( = and = ). Kepler-20b is a planet in a 3.7 day period with a mass of , resulting in a mean density of , indicating a rocky composition with an iron-to-silicate ratio consistent with that of the Earth. This makes Kepler-20b the most massive planet with a rocky composition found to date. Furthermore, we report the discovery of an additional non-transiting planet with a minimum mass of and an orbital period of ∼34 days in the gap between Kepler-20f ( P ∼ 11 days) and Kepler-20d ( P ∼ 78 days).

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.234

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.006
GPT teacher head0.191
Teacher spread0.185 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations89
Published2016
Admission routes1
Has abstractyes

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