An ultra-short-period super-Earth with an extremely high density and an outer companion

We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal. High precision radial velocity measurements from HARPS and HARPS-N confirm the transiting USP planet and reveal the existence of an outer (non-transiting) planet with an orbital period of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>∼</mml:mo></mml:math> 10 d. We measure a mass of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>7.67</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.75</mml:mn></mml:mrow> </mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo></mml:msub> </mml:math> and a radius of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>1.57</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.08</mml:mn></mml:mrow> </mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>R</mml:mi> <mml:mo>⊕</mml:mo></mml:msub> </mml:math> for the transiting planet, yielding a high mean density of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>11</mml:mn> <mml:mo>±</mml:mo> <mml:mn>2</mml:mn></mml:mrow> </mml:math> g <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msup><mml:mtext>cm</mml:mtext> <mml:mrow><mml:mo>-</mml:mo> <mml:mn>3</mml:mn></mml:mrow> </mml:msup> </mml:math> , making it the densest well-characterized USP super-Earth discovered to date. We measure a minimum mass of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>15.2</mml:mn> <mml:mo>±</mml:mo> <mml:mn>1.8</mml:mn></mml:mrow> </mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo></mml:msub> </mml:math> for the outer planet, and explore a migration formation pathway via the von Zeipel-Kozai-Lidov (ZKL) mechanism and tidal dissipation.

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Journal
Scientific Reports
Published
2024-11-08
DOI
https://doi.org/10.1038/s41598-024-76490-y
Citations
1
Primary Topic
Astro and Planetary Science
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article
Field-Weighted Citation Impact
0.33

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An ultra-short-period super-Earth with an extremely high density and an outer companion

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An ultra-short-period super-Earth with an extremely high density and an outer companion

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article en
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Abstract

We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal. High precision radial velocity measurements from HARPS and HARPS-N confirm the transiting USP planet and reveal the existence of an outer (non-transiting) planet with an orbital period of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>∼</mml:mo></mml:math> 10 d. We measure a mass of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>7.67</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.75</mml:mn></mml:mrow> </mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo></mml:msub> </mml:math> and a radius of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>1.57</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.08</mml:mn></mml:mrow> </mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>R</mml:mi> <mml:mo>⊕</mml:mo></mml:msub> </mml:math> for the transiting planet, yielding a high mean density of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>11</mml:mn> <mml:mo>±</mml:mo> <mml:mn>2</mml:mn></mml:mrow> </mml:math> g <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msup><mml:mtext>cm</mml:mtext> <mml:mrow><mml:mo>-</mml:mo> <mml:mn>3</mml:mn></mml:mrow> </mml:msup> </mml:math> , making it the densest well-characterized USP super-Earth discovered to date. We measure a minimum mass of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>15.2</mml:mn> <mml:mo>±</mml:mo> <mml:mn>1.8</mml:mn></mml:mrow> </mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>M</mml:mi> <mml:mo>⊕</mml:mo></mml:msub> </mml:math> for the outer planet, and explore a migration formation pathway via the von Zeipel-Kozai-Lidov (ZKL) mechanism and tidal dissipation.

Scientific ReportsVol. 14(1)
California Institute of Technology (US), Planetary Science Institute (US), University of Hawaii System (US), Okinawa Institute of Science and Technology Graduate University (JP), Universidad de La Laguna (ES), Lund University (SE), The Graduate University for Advanced Studies, SOKENDAI (JP), Aarhus University (DK), Nicolaus Copernicus University (PL), University of Oxford (GB), University of Chicago (US), Astrobiology Center (JP), Instituto de Astrofísica de Canarias (ES), Nicolaus Copernicus Astronomical Center (PL), Tokyo Metropolitan Komaba High School (JP), Thüringer Landessternwarte Tautenburg (DE), National Astronomical Observatory of Japan (JP), University College London (GB), McGill University (CA), University of Turin (IT), Keele University (GB), Chalmers University of Technology (SE), The University of Tokyo (JP)
National Science Foundation, National Aeronautics and Space Administration, NASA Exoplanet Science Institute, Vetenskapsrådet, Ministerio de Ciencia e Innovación, Uniwersytet Mikolaja Kopernika w Toruniu, Ames Research Center, Science Mission Directorate, Science and Technology Facilities Council, Japan Society for the Promotion of Science, European Regional Development Fund, Agencia Estatal de Investigación, Core Research for Evolutional Science and Technology
Openalex Percentile: Top 33%
Astro and Planetary Science
0.33
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