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Mark M. Phillips (born March 31, 1951) is an American astronomer who works on the observational studies of all classes of supernovae. He has worked on SN 1986G, SN 1987A, the Calán/Tololo Supernova Survey, the High-Z Supernova Search Team, and the Phillips relationship. This relationship has allowed the use of Type Ia supernovae as standard candles, leading to the precise measurements of the Hubble constant H0 and the deceleration parameter q0, the latter implying the existence of dark energy or a cosmological constant in the Universe.

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  • Mark M. Phillips (es)
  • Mark M. Phillips (en)
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  • Mark M. Phillips (nacido el 31 de marzo de 1951, San Diego, California, Estados Unidos) es internacionalmente reconocido astrónomo en los estudios observacionales de toda clase de supernova. Es muy conocido por su trabajo en SN1986G,​ SN 1987A,​ Proyecto Calán Tololo, el equipo de búsqueda de alta Z Supernova, y especialmente por la relación de Phillips.​​ Esta relación ha permitido el uso de la supernova de tipo Ia como candelas estándar, lo que lleva a las mediciones precisas de la constante de Hubble H0​​ y el parámetro de deceleración q0,​ el último que implica la existencia de la energía oscura o una constante cosmológica en el Universo. (es)
  • Mark M. Phillips (born March 31, 1951) is an American astronomer who works on the observational studies of all classes of supernovae. He has worked on SN 1986G, SN 1987A, the Calán/Tololo Supernova Survey, the High-Z Supernova Search Team, and the Phillips relationship. This relationship has allowed the use of Type Ia supernovae as standard candles, leading to the precise measurements of the Hubble constant H0 and the deceleration parameter q0, the latter implying the existence of dark energy or a cosmological constant in the Universe. (en)
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  • Mark M. Phillips (en)
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  • Mark M. Phillips (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/MMPhillipsIMG_7293x.jpg
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  • Mark M. Phillips (en)
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