Período27 jun 2015

Media contributions

1

Media contributions

  • TítuloV1191 Cygni
    Grau de reconhecimentoInternational
    Nome/saída de meios de comunicaçãoWikipedia
    Tipo de meios de comunicaçãoWeb
    PaísUnknown
    Data27/06/2015
    DescriçãoV1191 Cygni is the variable star designation for an overcontact binary star system in the constellation Cygnus.[12] First found to be variable in 1965, it is a W Ursae Majoris variable with a maximum apparent magnitude 10.82. It drops by 0.33 magnitudes during primary eclipses with a period of 0.3134 days, while dropping by 0.29 magnitudes during secondary eclipses.[10] The primary star, which is also the cooler star, appears to have a spectral type of F6V, while the secondary is slightly cooler with a spectral type of G5V.[3] With a mass of 1.29 solar masses and a luminosity of 2.71 solar luminosities, it is slightly more massive and luminous than the sun, while the secondary is only around 1/10 as massive and less than half as luminous. With a separation of 2.20 solar radii, the mass transfer of about 2×10−7 solar masses per year from the secondary to the primary is one of the highest known for a system of its type.[9]
    URLhttps://www.altmetric.com/details/4333223/wikipedia
    PessoasЕкатерина Анатольевна Аввакумова