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Telescope spies water plumes on dwarf planet Ceres - 0 views

  • Scientists
  • have made the first definitive detection of water vapor on the largest and roundest object in the asteroid belt, Ceres.
  • Plumes of water vapor are thought to shoot up periodically from Ceres when portions of its icy surface warm slightly
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  • Ceres is classified as a dwarf planet, a solar system body bigger than an asteroid and smaller than a planet.
  • "This is the first time water vapor has been unequivocally detected on Ceres or any other object in the asteroid belt and provides proof that Ceres has an icy surface and an atmosphere,"
  • Michael Küppers of ESA in Spain
  • NASA's Dawn mission, which is on its way to Ceres now after spending more than a year orbiting the large asteroid Vesta
  • Dawn is scheduled to arrive at Ceres in the spring of 2015, where it will take the closest look ever at its surface.
  • will map the geology and chemistry of the surface in high resolution
  • International Astronomical Union, the governing organization responsible for naming planetary objects
  • Ceres was known as the largest asteroid in our solar system
  • reclassified Ceres as a dwarf planet because of its large size. It is roughly 590 miles (950 kilometers) in diameter
  • When it first was spotted in 1801, astronomers thought it was a planet orbiting between Mars and Jupiter
  • Scientists believe Ceres contains rock in its interior with a thick mantle of ice that, if melted, would amount to more fresh water than is present on all of Earth
  • The materials making up Ceres likely date from the first few million years of our solar system's existence and accumulated before the planets formed.
  • Until now, ice had been theorized to exist on Ceres but had not been detected conclusively
  • far-infrared vision to see, finally, a clear spectral signature of the water vapor. But
  • did not see water vapor every time it looked
  • spied water vapor four different times, on one occasion there was no signature.
  • what scientists think is happening
  • when Ceres swings through the part of its orbit that is closer to the sun, a portion of its icy surface becomes warm enough to cause water vapor to escape in plumes
  • a rate of about 6 kilograms (13 pounds) per second
  • When Ceres is in the colder part of its orbit, no water escapes
  • The strength of the signal also varied over hours, weeks and months
  • water vapor plumes rotating in and out of Herschel's views as the object spun on its axis
  • This enabled the scientists to localize the source of water to two darker spots on the surface of Ceres
  • previously seen by NASA's Hubble Space Telescope and ground-based telescopes. The dark spots might be more likely to outgas because dark material warms faster than light material.
  • "The lines are becoming more and more blurred between comets and asteroids," said Seungwon Lee of JPL
  • Paul von Allmen, also of JPL. "We knew before about main belt asteroids that show comet-like activity, but this is the first detection of water vapor in an asteroid-like object."
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February 11 - Today in Science History - Scientists born on February 11th, died, and ev... - 0 views

  • Ceres observation interruption
  • In 1801, Giuseppe Piazzi made a 24th observation of the position of Ceres, the asteroid he discovered between the orbits of Mars and Jupiter, on 1 Jan 1801. It was the first and largest of the dwarf planets now known. After this, it moved into the light of the Sun, and was lost to view for most of the rest of the year. To mathematically relocate Ceres, Carl Gauss, age 24, took up the challenge to calculate its orbital path, based on the limited number of observations available. His method was tedious, requiring 100 hours of calculation. He began with a rough approximation for the unknown orbit, and then used it to produce a refinement, which became the subject of another improvement.. And so on. Astronomers using them found his results in close agreement as they located Ceres again 25 Nov-31 Dec 1801.«
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Curiosity Captures First Ever Asteroid Images from Mars Surface - 0 views

  • surface of the Red Planet during night sky imaging.
  • The Curiosity rover has captured the first images of asteroids even taken by a Human probe from the
  • two asteroids caught in the same night time pointing on the Red Planet. Namely, asteroids Ceres and Vesta.
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  • snapped by Curiosity’s high resolution Mastcam camera earlier this week on Sunday, April 20, 2014
  • whilst she was scanning about during daylight for her next drilling target at “The Kimberley” waypoint she pulled into at the start of this month.
  • Ceres and Vesta appear as streaks since the Mastcam image was taken as a 12 second time exposure.
  • “This imaging was part of an experiment checking the opacity of the atmosphere at night in Curiosity’s location on Mars, where water-ice clouds and hazes develop during this season,” said camera team member Mark Lemmon
  • “The two Martian moons were the main targets that night, but we chose a time when one of the moons was near Ceres and Vesta in the sky.”
  • Ceres, the largest asteroid, is about 590 miles (950 kilometers) in diameter. Vesta is the third-largest object in the main belt and measures about 350 miles (563 kilometers) wide.
  • the tinier of Mars’ moons, Deimos, was also caught in that same image.
  • Mars largest moon Phobos as well as massive planets Jupiter and Saturn were also visible that same Martian evening, albeit in a different pointing.
  • The two asteroids and three stars would be visible to someone of normal eyesight standing on Mars.
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Ceres (dwarf planet) - Wikipedia, the free encyclopedia - 0 views

  • in 1772, first suggested that an undiscovered planet could exist between the orbits of Mars and Jupiter
  • Kepler had already noticed the gap between Mars and Jupiter in 1596.
  • Giuseppe Piazzi at the Academy of Palermo
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  • discovered Ceres on 1 January 1801
  • Instead of a star, Piazzi had found a moving star-like object, which he first thought was a comet
  • Piazzi observed Ceres a total of 24 times, the final time on 11 February 1801, when illness interrupted his observations
  • The information was published in the September 1801
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Asteroid's troughs suggest stunted planet - 0 views

  • Scientists have been trying to determine the origin of these unusual troughs since their discovery just last year
  • new analysis supports the notion that the troughs are faults that formed when a fellow asteroid smacked into Vesta's south pole. The research reinforces the claim that Vesta has a layered interior, a quality normally reserved for larger bodies, such as planets and large moons.
  • ggest of those troughs, named Divalia Fossa, surpasses the size of the Grand Canyon by spanning 465 kilometers (289 miles) long, 22 km (13.6 mi) wide and 5 km (3 mi) deep
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  • The complexity of their formation can't be explained by simple collisions
  • New measurements
  • taken by NASA's Dawn spacecraft last year
  • indicate that a large collision could have created the asteroid's troughs
  • would only have been possible if the asteroid is differentiated – meaning that it has a core, mantle and crust
  • By saying it's differentiated, we're basically saying Vesta was a little planet trying to happen
  • previous research has found signs of igneous rock on Vesta, indicating that rock on Vesta's surface was once molten, a sign of differentiation
  • If the troughs are made possible by differentiation, then the cracks aren't just troughs, they're graben
  • graben is a dip in the surface that forms when two faults move apart from each other and the ground sinks into the widening gap
  • Vesta's troughs have many of the qualities of graben
  • observations indicate that Vesta is also unusually planet-like for an asteroid in that its mantle is ductile and can stretch under a lot of pressure
  • not yet fully convinced that Vesta's troughs are graben
  • There are other qualities of Vesta that could be clues to how the troughs formed
  • unlike the larger asteroid Ceres, Vesta is not classified as a dwarf planet because the large collision at its south pole knocked it out of its spherical shape
  • if Vesta has a mantle and core, that would mean it has qualities often reserved for planets, dwarf planets and moons—regardless of its shape
  • believes the south pole collision knocked Vesta into its current speedy rate of rotation about its axis of about once per 5.35 hours
  • may have caused the equator to bulge outward so far and so fast that the rotation caused the troughs, rather than the direct power of the impact
  • enigma why Vesta rotates so quickly
  • Dawn has already left to explore Ceres, so all the data it will retrieve on Vesta is in hand
  • scientists will continue to sort that data out and improve on computer simulations of Vesta's interior
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NASA to Reveal Vesta Discoveries by Dawn Asteroid Probe | Space.com - 0 views

  • NASA will showcase the latest discoveries from an asteroid probe orbiting the huge space rock Vesta on Thursday (May 10) in a press conference for reporters and the general public.
  • will present a new analysis of Vesta based on the latest observations from NASA's Dawn spacecraft
  • Dawn spacecraft launched in 2007 on a mission to visit two huge space rocks in the asteroid belt that orbits the sun between the orbits of Mars and Jupiter.
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  • Dawn arrived in orbit around Vesta in July 2011
  • Vesta is the brightest asteroid in the solar system and second most massive object in the asteroid belt
  • Last month, NASA extended Dawn's stay at Vesta by an extra 40 days to give the spacecraft more time to study the asteroid
  • spacecraft has revealed that many new details about Vesta
  • it is rich in iron and magnesium
  • experiences chilly temperatures that range from minus 10 degrees Fahrenheit (minus 23 degrees Celsius) in the sunlight, to minus150 degrees F (minus 100 degrees C) in shadowed areas.
  • Scientists think Vesta is a 4.5 billion-year-old relic left over from the formation of the solar system
  • In August the probe will move on to the Texas-size Ceres, the largest object in the asteroid belt and a space rock so large it is considered a dwarf planet.
  • expected to arrive at Ceres in February 2015
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