NOMINAL VALUES FOR SELECTED SOLAR AND PLANETARY QUANTITIES: IAU 2015 RESOLUTION B3

被引:313
作者
Prsa, Andrej [1 ]
Harmanec, Petr [2 ]
Torres, Guillermo [3 ]
Mamajek, Eric [4 ]
Asplund, Martin [5 ]
Capitaine, Nicole [6 ]
Christensen-Dalsgaard, Jorgen [7 ]
Depagne, Eric [8 ,9 ]
Haberreiter, Margit [10 ]
Hekker, Saskia [11 ,12 ]
Hilton, James [13 ]
Kopp, Greg [14 ]
Kostov, Veselin [15 ]
Kurtz, Donald W. [16 ]
Laskar, Jacques [17 ]
Mason, Brian D. [13 ]
Milone, Eugene F. [18 ]
Montgomery, Michele [19 ]
Richards, Mercedes [20 ]
Schmutz, Werner [10 ]
Schou, Jesper [21 ]
Stewart, Susan G. [13 ]
机构
[1] Villanova Univ, Dept Astrophys & Planetary Sci, 800 Lancaster Ave, Villanova, PA 19085 USA
[2] Charles Univ Prague, Fac Math & Phys, Astron Inst, V Holesovickach 2, CZ-18000 Prague 8, Czech Republic
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA
[5] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia
[6] Univ Paris 04, PSL Res Univ, Observ Paris, SYRTE,CNRS,UPMC,LNE, 61 Ave Observ, F-75014 Paris, France
[7] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
[8] South African Astron Observ, POB 9 Observ, Cape Town, South Africa
[9] Southern African Large Telescope, POB 9 Observ, Cape Town, South Africa
[10] World Radiat Ctr, Phys Meteorol Observ Davos, Dorfstr 33, Davos, Switzerland
[11] Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
[12] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
[13] US Naval Observ, 3450 Massachusetts Ave NW, Washington, DC 20392 USA
[14] Lab Atmospher & Space Phys, 1234 Innovat Dr, Boulder, CO 80303 USA
[15] NASA, Goddard Space Flight Ctr, Mail Code 665, Greenbelt, MD 20771 USA
[16] Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England
[17] UPMC, Observ Paris, CNRS, ASD IMCCE,PSL,UMR8028, 77 Ave Denfert Rochereau, F-75014 Paris, France
[18] Univ Calgary, Dept Phys & Astron, 2500 Univ Dr NW, Calgary, AB T2N 1N4, Canada
[19] Univ Cent Florida, Dept Phys, 4000 Cent Florida Blvd, Orlando, FL 32816 USA
[20] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[21] Max Planck Inst Solar Syst Res, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
基金
新加坡国家研究基金会; 美国国家科学基金会; 欧洲研究理事会;
关键词
planets and satellites: fundamental parameters; standards; stars: fundamental parameters; stars: general; Sun: fundamental parameters; ASTROPHYSICAL PARAMETERS; MODULES; CONSTANTS; ACCURACY; BINARIES; SET;
D O I
10.3847/0004-6256/152/2/41
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this brief communication we provide the rationale for. and the outcome of the International Astronomical Union (IAU) resolution vote at the XXIXth General Assembly in Honolulu, Hawaii, in 2015, on recommended nominal conversion constants for selected solar and planetary properties. The problem addressed by the resolution is a lack of established conversion constants between solar and planetary values and SI units: a missing standard has caused a proliferation of solar values (e.g., solar radius, solar irradiance, solar luminosity, solar effective temperature, and solar mass parameter) in the literature, with cited solar values typically based on best estimates at the time of paper writing. As precision of observations increases, a set of consistent values becomes increasingly important. To address this, an IAU Working Group on Nominal Units for Stellar and Planetary Astronomy formed in 2011, uniting experts from the solar, stellar, planetary, exoplanetary, and fundamental astronomy, as well as from general standards. fields to converge on optimal values for nominal conversion constants. The effort resulted in the IAU 2015 Resolution B3, passed at the IAU General Assembly by a large majority. The resolution recommends the use of nominal solar and planetary values, which are by definition exact and are expressed in SI units. These nominal values should be understood as conversion factors only, not as the true solar/planetary properties or current best estimates. Authors and journal editors are urged to join in using the standard values set forth by this resolution in future work and publications to help minimize further confusion.
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