GUARANTEE AUTHENTIC & BRAND NEW Silver, Gold -black Style #JF4482 Our striking Neptune's Ring's motif is flattened for a chic new take on a textured leather cuff bracelet. Width: 1 1/8' Closure: Magnetic hinged Length:, SM 7 1/2' Material: Leather Finish: Silver Gold plated Brighton Pouch or Tin isn't included Pictures may not show the true colors of the items. Most of the black spots.
Abstract: We report the discovery of a new planetary system with three transitingplanets, one super-Earth and two sub-Neptunes, that orbit EPIC,249893012, aG8,IV-V evolved star ($M_star$,=,1.05,$pm$,0.05,$M_odot$,$R_star$,=,1.71,$pm$,0.04,$R_odot$,$T_mathrm{eff}$,=5430,$pm$,85,K). The star is just leaving the mainsequence. We combined ktwo photometry with IRCS adaptive-optics imaging andHARPS, HARPS-N, and CARMENES high-precision radial velocity measurements toconfirm the planetary system, determine the stellar parameters, and measureradii, masses, and densities of the three planets. With an orbital period of$3.5949^{+0.0007}_{-0.0007}$ days, a mass of $8.75^{+1.09}_{-1.08} M_{oplus}$, and a radius of $1.95^{+0.09}_{-0.08} R_{oplus}$, the inner planet b iscompatible with nickel-iron core and a silicate mantle ($rho_b=6.39^{+1.19}_{-1.04}$ g cm$^{-3}$). Planets c and d with orbital periods of$15.624^{+0.001}_{-0.001}$ and $35.747^{+0.005}_{-0.005}$ days, respectively,have masses and radii of $14.67^{+1,84}_{-1.89} M_{oplus}$ and$3.67^{+0.17}_{-0.14} R_{oplus}$ and $10.18^{+2.46}_{-2.42} M_{oplus}$ and$3.94^{+0.13}_{-0.12} R_{oplus}$, respectively, yielding a mean density of$1.62^{+0.30}_{-0.29}$ and $0.91^{+0.25}_{-0.23}$ g cm$^{-3}$, respectively.The radius of planet b lies in the transition region between rocky and gaseousplanets, but its density is consistent with a rocky composition. Its semimajoraxis and the corresponding photoevaporation levels to which the planet has beenexposed might explain its measured density today. In contrast, the densitiesand semimajor axes of planets c and d suggest a very thick atmosphere. Thesingularity of this system, which orbits a slightly evolved star that is justleaving the main sequence, makes it a good candidate for a deeper study from adynamical point of view.
Submission history
Neptune 16 Sailboat
From: Diego Hidalgo Soto [view email][v1]Wed, 5 Feb 2020 12:33:36 UTC (1,970 KB)
Including brands such as Raid, Neptunes Harvest, Woodstock and Lawn-Boy. Mccormick Smoked Paprika 1.62 Oz (Pack 3) $22.82: Time left: 8h 15m. About the NEPTUNE 16 sailboat Calculations Help SA/Disp.: A sail area/displacement ratio below 16 would be considered under powered. 5.33 ft / 1.62 m P: 18.00 ft. Title: Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M$ oplus$ super-Earth and two warm 14.7 and 10.2-M$ oplus$ sub-Neptunes. And about duration - it is difficult to say, because every character has unique route. It usually takes me 1 hour to play 1 chapter for 1 character. So, if you are going to play all characters and all chapters - 20 hours. (sorry for my math:D ).
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Neptune 16 Review
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Bibliographic ToolsAbstract: We report the discovery of a new planetary system with three transitingplanets, one super-Earth and two sub-Neptunes, that orbit EPIC,249893012, aG8,IV-V evolved star ($M_star$,=,1.05,$pm$,0.05,$M_odot$,$R_star$,=,1.71,$pm$,0.04,$R_odot$,$T_mathrm{eff}$,=5430,$pm$,85,K). The star is just leaving the mainsequence. We combined ktwo photometry with IRCS adaptive-optics imaging andHARPS, HARPS-N, and CARMENES high-precision radial velocity measurements toconfirm the planetary system, determine the stellar parameters, and measureradii, masses, and densities of the three planets. With an orbital period of$3.5949^{+0.0007}_{-0.0007}$ days, a mass of $8.75^{+1.09}_{-1.08} M_{oplus}$, and a radius of $1.95^{+0.09}_{-0.08} R_{oplus}$, the inner planet b iscompatible with nickel-iron core and a silicate mantle ($rho_b=6.39^{+1.19}_{-1.04}$ g cm$^{-3}$). Planets c and d with orbital periods of$15.624^{+0.001}_{-0.001}$ and $35.747^{+0.005}_{-0.005}$ days, respectively,have masses and radii of $14.67^{+1,84}_{-1.89} M_{oplus}$ and$3.67^{+0.17}_{-0.14} R_{oplus}$ and $10.18^{+2.46}_{-2.42} M_{oplus}$ and$3.94^{+0.13}_{-0.12} R_{oplus}$, respectively, yielding a mean density of$1.62^{+0.30}_{-0.29}$ and $0.91^{+0.25}_{-0.23}$ g cm$^{-3}$, respectively.The radius of planet b lies in the transition region between rocky and gaseousplanets, but its density is consistent with a rocky composition. Its semimajoraxis and the corresponding photoevaporation levels to which the planet has beenexposed might explain its measured density today. In contrast, the densitiesand semimajor axes of planets c and d suggest a very thick atmosphere. Thesingularity of this system, which orbits a slightly evolved star that is justleaving the main sequence, makes it a good candidate for a deeper study from adynamical point of view.
Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.
Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs and how to get involved.
Bibliographic ToolsAbstract: We report the discovery of a new planetary system with three transitingplanets, one super-Earth and two sub-Neptunes, that orbit EPIC,249893012, aG8,IV-V evolved star ($M_star$,=,1.05,$pm$,0.05,$M_odot$,$R_star$,=,1.71,$pm$,0.04,$R_odot$,$T_mathrm{eff}$,=5430,$pm$,85,K). The star is just leaving the mainsequence. We combined ktwo photometry with IRCS adaptive-optics imaging andHARPS, HARPS-N, and CARMENES high-precision radial velocity measurements toconfirm the planetary system, determine the stellar parameters, and measureradii, masses, and densities of the three planets. With an orbital period of$3.5949^{+0.0007}_{-0.0007}$ days, a mass of $8.75^{+1.09}_{-1.08} M_{oplus}$, and a radius of $1.95^{+0.09}_{-0.08} R_{oplus}$, the inner planet b iscompatible with nickel-iron core and a silicate mantle ($rho_b=6.39^{+1.19}_{-1.04}$ g cm$^{-3}$). Planets c and d with orbital periods of$15.624^{+0.001}_{-0.001}$ and $35.747^{+0.005}_{-0.005}$ days, respectively,have masses and radii of $14.67^{+1,84}_{-1.89} M_{oplus}$ and$3.67^{+0.17}_{-0.14} R_{oplus}$ and $10.18^{+2.46}_{-2.42} M_{oplus}$ and$3.94^{+0.13}_{-0.12} R_{oplus}$, respectively, yielding a mean density of$1.62^{+0.30}_{-0.29}$ and $0.91^{+0.25}_{-0.23}$ g cm$^{-3}$, respectively.The radius of planet b lies in the transition region between rocky and gaseousplanets, but its density is consistent with a rocky composition. Its semimajoraxis and the corresponding photoevaporation levels to which the planet has beenexposed might explain its measured density today. In contrast, the densitiesand semimajor axes of planets c and d suggest a very thick atmosphere. Thesingularity of this system, which orbits a slightly evolved star that is justleaving the main sequence, makes it a good candidate for a deeper study from adynamical point of view.
Submission history
From: Diego Hidalgo Soto [view email][v1]Wed, 5 Feb 2020 12:33:36 UTC (1,970 KB)
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