Sonda Cassini inicia coleta de dados de uma das luas de Saturno [en]

A sonda Cassini, projeto conjunto da Nasa, Agência Espacial Européia e Agência Espacial da Itália iniciou, nesta quarta-feira (12), a coleta de dados no polo sul da lua Enceladus, de Saturno. A informação foi divulgada pelo Laboratório de Propulsão a Jato (JPL) da Nasa. Lançada no espaço em 15 de outubro de 1997, Cassini entrou na órbita de Saturno em 1° de Julho de 2004. É a primeira sonda a orbitar o planeta.

O instrumento foi deslocado a apenas 50 quilômetros do satélite natural, localizando-se numa região de gêiseres - nascente termal que entra em erupção periodicamente, lançando uma coluna de água quente e vapor para o ar, fonte de grande importância científica porque pode ser um indício de que existe água em forma líquida e até um oceano na região da lua. Os dados já estão sendo recebidos pela equipe espacial, a partir do recolhimento de pequenas partículas, de gelo, gás e poeira cósmica. 

Os instrumentos de análise da sonda determinarão as características químicas das partículas e estabelecerão o tamanho, a densidade e a composição destas. Já as câmeras instaladas transmitirão imagens até hoje nunca vistas em outras manobras da Cassini, nas cercanias da lua Enceladus.

Em 2005 os instrumentos de Cassini descobriram que os gêiseres do pólo sul da Enceladus chegam a uma distância três vezes maior que o raio da lua.

Cassini Spacecraft to Dive Into Water Plume of Saturn

The spacecraft, orchestrating its closest approach to date, will skirt along the edges of huge Old-Faithful-like geysers erupting from giant fractures on the south pole of Enceladus. Cassini will sample scientifically valuable water-ice, dust and gas in the plume.

The source of the geysers is of great interest to scientists who think liquid water, perhaps even an ocean, may exist in the area. While flying through the edge of the plumes, Cassini will be approximately 200 kilometers (120 miles) from the surface. At closest approach to Enceladus, Cassini will be only 50 kilometers (30 miles) from the moon.

"This daring flyby requires exquisite technical finesse, but it has the potential to revolutionize our knowledge of the geysers of Enceladus. The Cassini mission team is eager to see the scientific results, and so am I," said Alan Stern, associate administrator of NASA's Science Mission Directorate, Washington. 

Cassini's cameras will take a back seat on this flyby as the main focus turns to the spacecraft's particle analyzers that will study the composition of the plumes. The cameras will image Enceladus on the way in and out, between the observations of the particle analyzers.

Images will reveal northern regions of the moon previously not captured by Cassini. The analyzers will "sniff and taste" the plume. Information on the density, size, composition and speed of the gas and the particles will be collected.

"There are two types of particles coming from Enceladus, one pure water-ice, the other water-ice mixed with other stuff," said Sascha Kempf, deputy principal investigator for Cassini's Cosmic Dust Analyzer at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. "We think the clean water-ice particles are being bounced off the surface and the dirty water-ice particles are coming from inside the moon. This flyby will show us whether this concept is right or wrong."

In 2005, Cassini's multiple instruments discovered that this icy outpost is gushing water vapor geysers out to a distance of three times the radius of Enceladus. The moon is only 500 kilometers (310 miles) in diameter, but despite its petite size, it’s one of the most scientifically compelling bodies in our solar system. The icy water particles are roughly one ten-thousandth of an inch, or about the width of a human hair. The particles and gas escape the surface at jet speed at approximately 400 meters per second (800 miles per hour). The eruptions appear to be continuous, refreshing the surface and generating an enormous halo of fine ice dust around Enceladus, which supplies material to one of Saturn's rings, the E-ring.

Several gases, including water vapor, carbon dioxide, methane, perhaps a little ammonia and either carbon monoxide or nitrogen gas make up the gaseous envelope of the plume.

"We want to know if there is a difference in composition of gases coming from the plume versus the material surrounding the moon. This may help answer the question of how the plume formed," said Hunter Waite, principal investigator for Cassini's Ion and Neutral Mass Spectrometer at the Southwest Research Institute, San Antonio.

This is the first of four Cassini flybys of Enceladus this year. In June, Cassini completes its prime mission, a four-year tour of Saturn. Cassini's next flyby of Enceladus is planned for August, well into Cassini's proposed extended mission. Cassini will perform seven Enceladus flybys in its extended mission. If this encounter proves safe, future passes may bring the spacecraft even closer than this one. How close Cassini will be allowed to approach will be determined based on data from this flyby.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the Cassini-Huygens mission for NASA's Science Mission Directorate. The Cassini orbiter was designed, developed and assembled at JPL. (Nasa)