SETI Institute-Unistellar parceira promete revolucionar a astronomia amadora

19 de julho de 2017 -Mountain View, CA e Meyreuil, Françao Instituto SETI e a startup francesa Unistellar, anunciaram hoje uma parceria para comercializar um novo telescópio que promete oferecer uma visão incomparável do cosmos aos astrônomos amadores e oferecer a oportunidade de contribuir diretamente para ciência de ponta.

O novo eVscope™ da Unistellar aproveita a tecnologia de imagem “Enhanced Vision” e agora oferece três recursos únicos nunca antes oferecidos em um instrumento compacto de mercado de massa graças a esta parceria:

Observações de Dumbbell Nebula Messier 27, Whirlpool galaxy Messier 51 e Eagle Nebula Messier 16 usando um telescópio Unistellar do Observatoire des Baronnies Provençales, na França. Esta observação pode ser vista pelo usuário diretamente na lente e uma imagem pode ser gerada posteriormente para armazenamento na base de dados Unistellar no Instituto SETI.
Observações de Dumbbell Nebula Messier 27, Whirlpool galaxy Messier 51 e Eagle Nebula Messier 16 usando um telescópio Unistellar do Observatoire des Baronnies Provençales, na França. Esta observação pode ser vista pelo usuário diretamente na lente e uma imagem pode ser gerada posteriormente para armazenamento na base de dados Unistellar no Instituto SETI.

O Enhanced Vision produz imagens extremamente nitidas e detalhadas de objetos astronômicos até mesmo fracos, acumulando a luz e projetando-a na ocular do telescópio. A tecnologia Enhanced Vision imita a capacidade de coleta de luz de telescópios de refletor significativamente maiores, oferecendo visões sem precedentes de objetos do céu noturno anteriormente inacessíveis aos astrônomos amadores.  

Asociación de SETI Institute y Unistellar promete revolucionar astronomía amateur

SETI Institute y organización francesa Unistellar, anunciaron una asociación para comercializar un nuevo telescopio que promete entregar imágenes sin paralelo del cosmo a los astrónomos amateurs y proporcionar la oportunidad de contribuir de forma directa a ciencia de punta.

Nuevo eVscope™ de Unistelar eleva la tecnología de imagen “visión mejorada”  y proporciona tres características únicas nunca antes incluidas en instrumentos compactos para el mercado masivo, gracias a esta asociación.

Observar la nebulosa Messier 27, la galaxia Remolino Messier 51 y la nebulosa del Águila Messier 16 usando el telescopio Unistellar desde el observatorio des Baronnies Provençales, en Francia. Esta imagen puede verse directamente en el lente y una imagen puede generarse posteriormente para almacenarse en la base de datos Unistellas en SETI Institute.
Observar la nebulosa Messier 27, la galaxia Remolino Messier 51 y la nebulosa del Águila Messier 16 usando el telescopio Unistellar desde el observatorio des Baronnies Provençales, en Francia. Esta imagen puede verse directamente en el lente y una imagen puede generarse posteriormente para almacenarse en la base de datos Unistellas en SETI Institute.

SETI Alumni: Portrait of Sarah Blunt

SETI Institute GPI group from left to right: Eric Nielsen, Franck Marchis, Jasmine Garani, Sarah Blunt, and Clement Chalumeau
SETI Institute GPI group from left to right: Eric Nielsen, Franck Marchis, Jasmine Garani, Sarah Blunt, and Clement Chalumeau (credit: F. Marchis/SETI Institute)

Sarah Blunt, REU student class of 2015, is today a full member of the Gemini Planet Imager Exoplanet Survey. Together with SETI researcher Eric Nielsen and Franck Marchis, she has developed an innovative method to fit the orbits of directly imaged exoplanets. She has published her work in Astronomical Journal and is a recipient of an NSF Graduate Research Fellowship that will fund her graduate school. Here her story.

Director of the Carl Sagan Center of the SETI Institute publishes a Carl Sagan Biographical Memoir

David Morrison, director of the Carl Sagan Center of the SETI Institute, has written a biographical memoir of Carl Sagan (1934-1996), founder of the modern disciplines of planetary science and exobiology.

Carl Sagan (third from left) with three of his former students: David Morrison, Joseph Veverka, and James Pollack. Photo by David Morrison
Carl Sagan (third from left) with three of his former students: David Morrison, Joseph Veverka, and James Pollack. Photo by David Morrison

Meeting the Team: GPI Science Meeting November 2013

The Gemini Planet Imager (GPI) team held our latest science meeting November 1-2, 2013, right before GPI saw first starlight. The meeting was hosted by the SETI Institute at their office in Mountain View, CA (for those curious, I did not find any signs of aliens there). Continuing with tradition, we took a group picture of the GPI team. You can tell it has grown significantly from the past.

Group picture taken at the GPI Science Meeting in November 2013.
Group picture taken at the GPI Science Meeting in November 2013.

GPI is ready for its new location in Chile

It is now official, The Gemini Planet Imager (“Gee-pi”) is ready for shipping to Chile. This decision was taken on July 19 after the positive pre-delivery acceptance review. From its current home at the University of California Santa Cruz, the instrument’s Integral Field Spectrograph (IFS) began its warm-up a week later (July 25th), and the computers were shut-down two days ago (July 31st).

Ifs_install
The Integral Field Spectrograph (the “eye” of GPI) being installed in the GPI instrument (archive picture from 2012)

GPI is going to be carefully packed for a long trip to Chile. The instrument will be shipped to the southern hemisphere by plane and should arrive by the end of August.

Featuring the Women Of Science #WomenOfScience

Today I would like to share with you an idea for the International Women’s day on March 8 2013.  If you work in an institution, university, or non-profit related to science, have you taken note of the number of women around you? In astronomy and planetary science, it is not too bad even if it is not perfect, but some “hard” science groups, like physics or computer science, clearly have a low proportion of women in their ranks. I will not elaborate on the reasons for such lack of representation; instead, I propose to focus on the bright side.