NAOC Open IR
HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS
Gan, Tianjun1; Bedell, Megan2; Wang, Sharon Xuesong1; Foreman-Mackey, Daniel2; Melendez, Jorge3; Mao, Shude1,4; Stassun, Keivan G.5,6; Howell, Steve B.7; Ziegler, Carl8; Wittenmyer, Robert A.9; Hellier, Coel10; Collins, Karen A.11; Shporer, Avi12,13; Ricker, George R.12,13; Vanderspek, Roland12,13; Latham, David W.11; Seager, Sara12,13,14,15; Winn, Joshua N.16; Jenkins, Jon M.7; Addison, Brett C.9; Ballard, Sarah17; Barclay, Thomas18,19; Bean, Jacob L.20; Bowler, Brendan P.21; Briceno, Cesar22; Crossfield, Ian J. M.23; Dittman, Jason11,24; Horner, Jonathan9; Jensen, Eric L. N.25; Kane, Stephen R.26; Kielkopf, John27; Kreidberg, Laura11,24; Law, Nicholas28; Mann, Andrew W.28; Mengel, Matthew W.9; Morgan, Edward H.12,13; Okumura, Jack9; Osborn, Hugh P.12,13,29; Paegert, Martin11; Plavchan, Peter30; Schwarz, Richard P.31; Shiao, Bernie32; Smith, Jeffrey C.7,33; Spina, Lorenzo34; Tinney, C. G.35; Torres, Guillermo11; Twicken, Joseph D.7,33; Vezie, Michael12,13; Wang, Gavin36,37; Wright, Duncan J.9; Zhang, Hui38
2021-10-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume507Issue:2Pages:2220-2240
AbstractWe report the discovery and characterization of a transiting warm sub-Neptune planet around the nearby bright (V = 8.75 mag, K = 7.15 mag) solar twin HD 183579, delivered by the Transiting Exoplanet Survey Satellite (TESS). The host star is located 56.8 +/- 0.1 pc away with a radius of R-* = 0.97 +/- 0.02R(circle dot) and a mass of M-* = 1.03 +/- 0.05M(circle dot). We confirm the planetary nature by combining space and ground-based photometry, spectroscopy, and imaging. We find that HD 183579b (TOI-1055b) has a radius of R-p = 3.53 +/- 0.13R(circle plus) on a 17.47 d orbit with a mass of M-p = 11.2 +/- 5.4M(circle plus) (3 sigma mass upper limit of 27.4M(circle plus)). HD 183579b is the fifth brightest known sub-Neptune planet system in the sky, making it an excellent target for future studies of the interior structure and atmospheric properties. By performing a line-by-line differential analysis using the high-resolution and signal-to-noise ratio HARPS spectra, we find that HD 183579 joins the typical solar twin sample, without a statistically significant refractory element depletion.
Keywordplanets and satellites: detection planets and satellites: gaseous planets planets and satellites: individual: (HD 183579, HIP 96160, TIC 320004517, TOI 1055) stars: abundances stars: solar type
Funding OrganizationNational Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes ; National Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes ; National Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes ; National Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes
DOI10.1093/mnras/stab2224
WOS KeywordERROR-CORRECTION ; GALACTIC THIN ; PLANET SEARCH ; M-DWARF ; STARS ; MASS ; PERIODOGRAM ; VELOCITIES ; SIGNATURES ; TELESCOPE
Language英语
Funding ProjectNational Science Foundation of China[11390372] ; National Science Foundation of China[11761131004] ; FAPESP[2018/04055-8] ; NSFC[12073010] ; Swiss National Science Foundation ; SNSF ; NASA's Science Mission directorate ; European Southern Observatory[188.C-0265] ; European Southern Observatory[0100.D-0444] ; Australian Research Council[LE160100001] ; Australian Research Council[DP180100972] ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; UNSW Sydney ; MIT ; Nanjing University ; George Mason University ; University of Louisville ; University of California Riverside ; University of Florida ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; TAP member institutes
Funding OrganizationNational Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes ; National Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes ; National Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes ; National Science Foundation of China ; National Science Foundation of China ; FAPESP ; FAPESP ; NSFC ; NSFC ; Swiss National Science Foundation ; Swiss National Science Foundation ; SNSF ; SNSF ; NASA's Science Mission directorate ; NASA's Science Mission directorate ; European Southern Observatory ; European Southern Observatory ; Australian Research Council ; Australian Research Council ; Mount Cuba Astronomical Foundation ; Mount Cuba Astronomical Foundation ; University of Southern Queensland ; University of Southern Queensland ; UNSW Sydney ; UNSW Sydney ; MIT ; MIT ; Nanjing University ; Nanjing University ; George Mason University ; George Mason University ; University of Louisville ; University of Louisville ; University of California Riverside ; University of California Riverside ; University of Florida ; University of Florida ; University of Texas at Austin ; University of Texas at Austin ; NASA Exoplanet Exploration Program ; NASA Exoplanet Exploration Program ; TAP member institutes ; TAP member institutes
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000697380800044
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/75013
Collection中国科学院国家天文台
Corresponding AuthorGan, Tianjun; Wang, Sharon Xuesong
Affiliation1.Tsinghua Univ, Dept Astron & Tsinghua, Ctr Astrophys, Beijing 100084, Peoples R China
2.Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USA
3.Univ Sao Paulo, Dept Astron, IAG, Rua Matao 1226, BR-05509900 Sao Paulo, Brazil
4.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
5.Vanderbilt Univ, Dept Phys & Astron, 6301 Stevenson Ctr Ln, Nashville, TN 37235 USA
6.Fisk Univ, Dept Phys, 1000 17th Ave North, Nashville, TN 37208 USA
7.NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
8.Stephen F Austin State Univ, Dept Phys Engn & Astron, 1936 North St, Nacogdoches, TX 75962 USA
9.Univ Southern Queensland, Ctr Astrophys, West St, Toowoomba, Qld 4350, Australia
10.Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England
11.Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA
12.MIT, Dept Phys, Cambridge, MA 02139 USA
13.MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
14.MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
15.MIT, Dept Aeronaut & Astronaut, 77 Massachusetts Ave, Cambridge, MA 02139 USA
16.Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA
17.Univ Florida, Depariment Astron, 211 Bryant Space Sci Ctr, Gainesville, FL 32611 USA
18.NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
19.Univ Maryland, 1000 Hilltop Circle, Baltimore, MD 21250 USA
20.Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
21.Univ Texas Austin, Dept Astron, Austin, TX 78712 USA
22.Cerro Tololo Interamer Observ, Carina 603, La Serena, Chile
23.Univ Kansas, Dept Phys & Astron, 1082 Malott,1251 Wescoe Hall Dr, Lawrence, KS 66045 USA
24.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
25.Swarthmore Coll, Dept Phys & Astron, Swarthmore, PA 19081 USA
26.Univ Calif Riverside, Dept Earth & Planetary Sci, Riverside, CA 92521 USA
27.Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA
28.Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA
29.Univ Bern, Ctr Space & Habitabil, NCCR PlanetS, CH-3012 Bern, Switzerland
30.George Mason Univ, 4400 Univ Dr MS 3F3, Fairfax, VA 22030 USA
31.Patashnick Voorheesville Observ, Voorheesville, NY 12186 USA
32.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
33.SETI Inst, 189 Bernardo Ave,Suite 200, Mountain View, CA 94043 USA
34.INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
35.UNSW Sydney, Sch Phys, Exoplanetary Sci UNSW, Sydney, NSW 2052, Australia
36.Tsinghua Int Sch, Beijing 100084, Peoples R China
37.StanfordOnline High Sch, 415 Broadway Acad Hall,Floor 2,8853, Redwood City, CA 94063 USA
38.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Sch Astron & Space Sci, Nanjing 210046, Jiangsu, Peoples R China
Recommended Citation
GB/T 7714
Gan, Tianjun,Bedell, Megan,Wang, Sharon Xuesong,et al. HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,507(2):2220-2240.
APA Gan, Tianjun.,Bedell, Megan.,Wang, Sharon Xuesong.,Foreman-Mackey, Daniel.,Melendez, Jorge.,...&Zhang, Hui.(2021).HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,507(2),2220-2240.
MLA Gan, Tianjun,et al."HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 507.2(2021):2220-2240.
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