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TOPIC: ESApod


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RE: ESApod
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ROSE_S.jpg
spacer.gifAsteroid Steins belongs to the rare, largely unknown intermediate E-class, very bright and probably with a much-weathered surface. Steins' orbit was only known from ground observations, so Rosetta is conducting Europe's first-ever optical tracking campaign, providing highly accurate position data to Flight Dynamics specialists who are planning a series of trajectory corrections for an accurate fly-by. For over a year, Rosetta scientists and leading asteroid experts have been planning this encounter, and all the probe's science instruments will be active at some point in the fly-by. Reception of the first images is expected at the European Space Operations Centre some two hours after the encounter on 5 September 2008.

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spacer.gifSteins is Rosetta's first nominal scientific target. Based upon ground-based observations, it has been classified as an 'E-type' asteroid, composed mainly of silicates and basalts, but its properties are not known in detail. For these reasons, it has been selected as one of the two asteroids that Rosetta will study, from among those that were within reach of the mission. The study of asteroids is extremely important as they represent a sample of Solar System material at different stages of evolution key to understanding the origin of our own planet and of our planetary neighbourhood. The spacecraft will rendezvous with the asteroid in the course of its first incursion into the asteroid belt, while on its way to comet 67/P Churyumov-Gerasimenko.

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spacer.gifThe search for water in space has been quite successful; traces of ice have been found on Mars and water vapour has been found in several places in our galaxy. Water vapour was also recently detected on a planet outside our Solar System for the first time. It was an important discovery, although the planet is far too hot to be able to support life. Heavy water, which is also found on comets, poses the question of whether we can trace the origins of the water on earth through the heavy water found on objects like asteroids and comets. The Herschel space observatory, due for launch within a years time, will help explore the theory that water vapour plays an important role in regions of space where interstellar clouds of gas and dust are forming new stars.

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spacer.gifHubble has been serviced and upgraded four times. The fifth and final tune-up is scheduled for October 2008. After this, it is expected to be in fit working order for another five years. The James Webb Space Telescope (JWST), a project of partnership between ESA, NASA and the Canadian Space Agency, is scheduled for launch in 2013. It is the largest and most complex space probe ever built. JWST will observe in infrared wavelengths, providing unprecedented results.

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Ulysses_S.jpg
spacer.gifFor more than 17 years, the joint ESA/NASA mission Ulysses studied the heliosphere (the sphere of influence of the Sun) and our local interstellar neighbourhood, providing the first-ever map of the heliosphere in the four dimensions of space and time. Ulysses was designed to last for five years but it is still returning valuable data. The mission, which takes the spacecraft over the poles of the Sun, was extended four times, allowing Ulysses to pass over the Suns poles for a second and third time. But like all good things, the mission is coming to an end.

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Galileo, time and space
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spacer.gifThe Galileo constellation will be the world's most reliable global navigation system. The technologies that have been developed to achieve such precision will also provide data for use in many other fields, such as oceanography and meteorology. The Galileo system will also open new horizons in fundamental sciences. The extremely small differences in timekeeping between the satellite clocks moving in orbit and their Earth-bound counterparts will lead scientists to a re-evaluation of the nature and influence of gravity in the Universe.

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Earth Observation highlights at ILA Space Pavilion
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spacer.gifEarlier this week, ESA signed a contract at the Berlin Airshow's Space Pavilion to build the EarthCARE satellite - the Agency's 'Cloud, Aerosol and Radiation' mission. Due for launch in 2013, EarthCARE will gather data to give scientists a better understanding of the interactions between radiation and clouds and aerosols in the atmosphere. Earth Observation is a central pillar in Europe's space activities; EO generates direct benefits for citizens and governments and employs science for a better understanding of our planet.

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Mars_S.jpg
spacer.gifRadar sounders aboard ESAs Mars Express and NASAs Mars Reconnaissance orbiters have already detected ice deposits deep underground. Now, after a ten-month journey, NASAs Phoenix lander will continue the search for water. Its objective is to land in a permafrost region near the north pole. Its suite of instruments will scan the atmosphere and a robotic arm will attempt to dig down to an ice-rich layer expected to lie at arms reach below the surface. But water is not the sole element that could have harboured life on the Red Planet: methane could also establish a link between life on Earth and Mars. Scientists have already found traces of methane in the atmosphere of Mars and are currently trying to work out exactly where the gas is coming from. On Earth, it is well known that the source of methane is mostly life. So, whilst orbiting spacecraft like Mars Express continue to harvest global views, in-situ observations on the martian surface like those of NASAs Phoenix lander and ESAs ExoMars mobile laboratory, due to launch in 2011, remain necessary. The critical entry, descent and landing phase of the Phoenix probe will, at NASAs request, be provided with support from ESA.

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spacer.gifFrom an exceptionally low orbital altitude, GOCE (Gravity Field and steady-state Ocean Circulation Explorer) will measure global variations in the Earth's gravity field with extreme detail and accuracy. This will result in a unique model of the geoid, which is the surface of equal gravitational potential defined by the gravity field crucial for deriving accurate measurements of ocean circulation and sea-level change, both of which are affected by climate change. GOCE-derived data is also much needed to understand more about processes occurring inside the Earth and for use in practical applications such as surveying and levelling. GOCE is the first in the series of Earth Explorer missions being developed within ESA's Living Planet Programme. Earth Explorer missions form the science and research element of the Living Planet Programme and focus on the atmosphere, biosphere, hydrosphere, cryosphere and the Earth's interior, with the overall emphasis on learning more about the interactions between these components and the impact that human activity is having on natural Earth processes. The satellite is currently undergoing final preparations at ESA-ESTEC in the Netherlands prior to launch this summer from the Plesetsk Cosmodrome in northern Russia.

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spacer.gifThe advantage of using leading edge-technologies from space in other sectors, and vice versa, at the forum 'Innovation from space exploration and technology transfer' taking place 23 April 2008.

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