Gliese 588

Gliese 588
	estrella variable, fonte d'infrarroxos, fuente astrofísica de rayos X (es) , estrella con movimiento propio alto (es) y near-IR source (en)
Datos d'observación
Ascensión reuta (α)	233,05388462876 °
Declinación (δ)	−41,27559178719 °
Distancia a la Tierra	5,9172 pc
Magnitú aparente (V)	9,311 (banda V)
Magnitú absoluta	10,41
Constelación	Lobo (es)
Velocidá de rotación	2,4 km/s
Velocidá radial	21,459 km/s
Parallax	168,9965 mas
Carauterístiques físiques
Masa	0,44 M☉
Gravedá superficial	58 000 cm/s²
Tipu espectral	M5
Otros nomes
	Ver llista PLX 3501 (General Catalogue of Trigonometric Stellar Parallaxes (es) ); GJ 588 (Catálogu Gliese); HIC 76074 (Hipparcos Input Catalogue (en) ); HIP 76074 (Catálogu Hipparcos); IRAS 15288-4106 (IRAS (es) ); LFT 1208 (Luyten Five-Tenths catalogue (en) ); LHS 397 (Luyten Half-Second catalogue (en) ); LTT 6210 (Luyten Two-Tenths catalogue (en) ); NLTT 40449 (New Luyten Two-Tenths catalogue (en) ); NSV 7119 (New Catalogue of Suspected Variable Stars (es) ); Zkh 218 (Catálogo Zakhozhaj (es) ); 2MASS J15321302-4116314 (2MASS (es) ); PLX 3501.00 (General Catalogue of Trigonometric Stellar Parallaxes (es) ); 1RXS J153212.5-411640 (1RXS (en) ); PM 15290-4105 (Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more (en) ); CF 13312 (Catalogue of 20554 faint stars in the Cape astrographic zone -40 to -52 for the equinox of 1900.0, Royal Obs. Cape of Good Hope (en) ); Ci 20 934 (Catalogue of proper motion stars (en) ); RX J1532.2-4116 (X-ray survey of the Large Magellanic Cloud by ROSAT (en) ); PM J15322-4116 (Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more (en) ); Gaia DR2 6002807341299977216 (Gaia DR2 (es) ); TIC 149590989 (TESS Input Catalog (en) ); Gaia DR3 6002807341299977216 (Gaia DR3 (es) ); TYC 7844-1976-1 (Tycho Catalogue (en) ); UBV M 6108 (UBV Photoelectric Photometry Catalogue (en) );

Gliese 588 o GJ 588 (LHS 397 / CD-40 9712 / HIP 76074)^[9] ye una estrella na constelación de Lupus, el llobu, alcontrada visualmente a 34 minutos d'arcu al oeste de la brillosa γ Lupi. Asitiada a 19,36 años lluz de distancia, ye la estrella más próxima al Sol nesta constelación.

Coordenaes: 15^h 32^m 12.932^s, -41^° 16^′ 32.13^″

Gliese 588 ye una nana colorada de tipu espectral M3.0V y magnitú aparente +9,31.^[10] Tien una masa igual al 46% de la masa solar^[10] y un radiu equivalente al 48% del que tien el Sol.^[11] La so lluminosidá namái supón el 4% de la lluminosidá solar y la so temperatura efectivo ye de 3440 K.^[12] Como posible estrella variable, recibe la denominación NSV 7119 nel New Catalogue of Suspected Variable Stars. En concretu, la midida del so índiz d'actividá magnética per aciu el doblete de la llinia NaI de la so espectru, punxo de manifiestu que dicha actividá varia nuna escala de tiempu llarga; amás, esiste una correllación significativa ente l'actividá de la estrella y les variaciones de la so velocidá radial.^[13]

La estrelles conocíes más cercanes a Gliese 588 son GJ 3877, nana colorada a 5,4 años lluz, y Gliese 570, sistema estelar a 7,1 años lluz.^[14]

Ver tamién

Llista d'estrelles cercanes a la Tierra

Referencies

↑ ^1,0 ^1,1 ^1,2 ^1,3 ^1,4 Afirmao en: SIMBAD.
↑ ^2,0 ^2,1 ^2,2 ^2,3 Afirmao en: Gaia EDR3. Stated in source according to: SIMBAD. Llingua de la obra o nome: inglés. Data d'espublización: 3 avientu 2020.
↑ ^3,0 ^3,1 URL de la referencia: http://wwwadd.zah.uni-heidelberg.de/datenbanken/aricns/cnspages/4c01221.htm.
↑ «The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations». Astronomy and Astrophysics: páxs. 20. xunetu 2020. doi:10.1051/0004-6361/202038035.
↑ Caroline Soubiran (agostu 2018). «Gaia Data Release 2. The catalogue of radial velocity standard stars» (n'inglés). Astronomy and Astrophysics. doi:10.1051/0004-6361/201832795.
↑ Afirmao en: Wikipedia en polaco. Llingua de la obra o nome: polacu.
↑ J. Maldonado (avientu 2020). «HADES RV programme with HARPS-N at TNG. XII. The abundance signature of M dwarf stars with planets» (n'inglés). Astronomy and Astrophysics: páxs. 23. doi:10.1051/0004-6361/202039478.
↑ «New "weak-line"-T Tauri stars in Lupus». Astronomy and Astrophysics: páxs. 329–352. 1997. doi:10.1051/AAS:1997163.
↑ GJ 588 -- Variable Star (SIMBAD)
↑ ^10,0 ^10,1 The One Hundred Nearest Star Systems (RECONS)
↑ Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (2001). «Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics». Astronomy and Astrophysics 367. páxs. 521-524. http://cdsarc.u-strasbg.fr/cgi-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=12824.
↑ Morales, J. C.; Ribas, I.; Jordi, C. (2008). «The effect of activity on stellar temperatures and radii». Astronomy and Astrophysics 478 (2). páxs. 507-512. http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2008A%26A...478..507M&db_key=AST&nosetcookie=1.
↑ Gomes da Silva, J.; Santos, N. C.; Bonfils, X.; Delfosse, X.; Forveille, T.; Udry, S.; Dumusque, X.; Lovis, C. (2012). «Long-term magnetic activity of a sample of M-dwarf stars from the HARPS program . II. Activity and radial velocity». Astronomy and Astrophysics 541. A9. http://adsabs.harvard.edu/cgi-bin/nph-bib_query?2012A%26A...541A...9G&db_key=AST.
↑ Cordoba Durchmusterung -40°9712 (The Internet Stellar Database)

Coordenaes: 15^h 32^m 12.932^s, -41^° 16^′ 32.13^″

[8ba559d5760a03bedaaacc3c347bbfe4981560bf-1] 1,0 ^1,1 ^1,2 ^1,3 ^1,4 Afirmao en: SIMBAD.

[88f46fab9cce60c7e274ff942763157775017282-2] 2,0 ^2,1 ^2,2 ^2,3 Afirmao en: Gaia EDR3. Stated in source according to: SIMBAD. Llingua de la obra o nome: inglés. Data d'espublización: 3 avientu 2020.

[8a2c3c088d2362c455223a3c87a09c26c0d4f00f-3] 3,0 ^3,1 URL de la referencia: http://wwwadd.zah.uni-heidelberg.de/datenbanken/aricns/cnspages/4c01221.htm.

[841fd48f3d301a0e7ebf73a6e8e30c4fd98a03b9-4] «The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations». Astronomy and Astrophysics: páxs. 20. xunetu 2020. doi:10.1051/0004-6361/202038035.

[3bf3b74f599a0eb91eecfea10ab3e78fe4e80b5e-5] Caroline Soubiran (agostu 2018). «Gaia Data Release 2. The catalogue of radial velocity standard stars» (n'inglés). Astronomy and Astrophysics. doi:10.1051/0004-6361/201832795.

[199c244198f785d02f28294dcd79b3a37d5670fc-6] Afirmao en: Wikipedia en polaco. Llingua de la obra o nome: polacu.

[aa3096a7b63d5ced9b46d26453fa5bc89db4cc20-7] J. Maldonado (avientu 2020). «HADES RV programme with HARPS-N at TNG. XII. The abundance signature of M dwarf stars with planets» (n'inglés). Astronomy and Astrophysics: páxs. 23. doi:10.1051/0004-6361/202039478.

[1eb044e5b854a79790314c1b916c5c6c975b32a6-8] «New "weak-line"-T Tauri stars in Lupus». Astronomy and Astrophysics: páxs. 329–352. 1997. doi:10.1051/AAS:1997163.

[9] GJ 588 -- Variable Star (SIMBAD)

[RECONS-10] 10,0 ^10,1 The One Hundred Nearest Star Systems (RECONS)

[11] Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (2001). «Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics». Astronomy and Astrophysics 367. páxs. 521-524. http://cdsarc.u-strasbg.fr/cgi-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=12824.

[Morales-12] Morales, J. C.; Ribas, I.; Jordi, C. (2008). «The effect of activity on stellar temperatures and radii». Astronomy and Astrophysics 478 (2). páxs. 507-512. http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2008A%26A...478..507M&db_key=AST&nosetcookie=1.

[Gomes-13] Gomes da Silva, J.; Santos, N. C.; Bonfils, X.; Delfosse, X.; Forveille, T.; Udry, S.; Dumusque, X.; Lovis, C. (2012). «Long-term magnetic activity of a sample of M-dwarf stars from the HARPS program . II. Activity and radial velocity». Astronomy and Astrophysics 541. A9. http://adsabs.harvard.edu/cgi-bin/nph-bib_query?2012A%26A...541A...9G&db_key=AST.

[14] Cordoba Durchmusterung -40°9712 (The Internet Stellar Database)

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Gliese 588
estrella variable^[1], fonte d'infrarroxos^[1], fuente astrofísica de rayos X ^(es) ^[1], estrella con movimiento propio alto ^(es) ^[1] y near-IR source ^(en) ^[1]
Datos d'observación
Ascensión reuta (α)	233,05388462876 °^[2]
Declinación (δ)	−41,27559178719 °^[2]
Distancia a la Tierra	5,9172 pc
Magnitú aparente (V)	9,311 (banda V)
Magnitú absoluta	10,41^[3]
Constelación	Lobo ^(es)
Velocidá de rotación	2,4 km/s^[4]
Velocidá radial	21,459 km/s^[5]
Parallax	168,9965 mas^[2]
Carauterístiques físiques
Masa	0,44 M☉^[6]
Gravedá superficial	58 000 cm/s²^[7]
Tipu espectral	M5^[8]
Otros nomes
Ver llista PLX 3501 (General Catalogue of Trigonometric Stellar Parallaxes ^(es) ) GJ 588 (Catálogu Gliese) HIC 76074 (Hipparcos Input Catalogue ^(en) ) HIP 76074 (Catálogu Hipparcos) IRAS 15288-4106 (IRAS ^(es) ) LFT 1208 (Luyten Five-Tenths catalogue ^(en) ) LHS 397 (Luyten Half-Second catalogue ^(en) ) LTT 6210 (Luyten Two-Tenths catalogue ^(en) ) NLTT 40449 (New Luyten Two-Tenths catalogue ^(en) ) NSV 7119 (New Catalogue of Suspected Variable Stars ^(es) ) Zkh 218 (Catálogo Zakhozhaj ^(es) ) 2MASS J15321302-4116314 (2MASS ^(es) ) PLX 3501.00 (General Catalogue of Trigonometric Stellar Parallaxes ^(es) ) 1RXS J153212.5-411640 (1RXS ^(en) ) PM 15290-4105 (Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more ^(en) ) CF 13312 (Catalogue of 20554 faint stars in the Cape astrographic zone -40 to -52 for the equinox of 1900.0, Royal Obs. Cape of Good Hope ^(en) ) Ci 20 934 (Catalogue of proper motion stars ^(en) ) RX J1532.2-4116 (X-ray survey of the Large Magellanic Cloud by ROSAT ^(en) ) PM J15322-4116 (Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more ^(en) ) Gaia DR2 6002807341299977216 (Gaia DR2 ^(es) ) TIC 149590989 (TESS Input Catalog ^(en) ) Gaia DR3 6002807341299977216 (Gaia DR3 ^(es) ) TYC 7844-1976-1 (Tycho Catalogue ^(en) ) UBV M 6108 (UBV Photoelectric Photometry Catalogue ^(en) )