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Destination Tomorrow - DT6 - Mars Exploration
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NASA Destination Tomorrow Segment highlighting NASA's contemporary exploration of Mars.
For hundreds of years, humans have dreamed of exploring the planet Mars.
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One important reason for this is that, other than Earth, Mars is the planet with the most
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hospitable climate in our solar system.
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The climate on Mars is so hospitable, in fact, that many scientists believe that liquid water
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may have once flowed over its surface, harboring primitive bacterial life.
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In an effort to investigate these intriguing possibilities, NASA's planned several new
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Mars exploration missions.
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NASA planners hope these missions will help explain many unanswered questions about the
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Red Planet and how those answers will affect us here on Earth.
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I spoke with Preysan Desai from NASA Langley Research Center to find out more.
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In mid-2003, two Mars exploration rovers will be launched to explore the surface of Mars.
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You may remember the Pathfinder mission from a few years ago.
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These are very similar, but have some major differences.
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The Pathfinder mission had a lander, which acted as a base station, and a small rover,
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which was about a foot and a half in length.
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The 2003 rovers have many more instruments and will be able to traverse much longer distances
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on the surface of Mars.
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These new rovers will act like mobile field geologists.
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This mission is actually very exciting compared to previous missions.
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For the first time, the rovers will be able to go much greater distances away from the
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lander, and for the first time, we could also go to a hill on top of it and see what's
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over it.
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And so, we would be able to cover a lot more different areas and see different geological
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features to try to get a better understanding of how Mars is evolving in those regions.
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Preysan, what's the process of getting the rovers to Mars?
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Well, Tonya, the rovers will be launched on Delta rockets in June and July of 2003.
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The rockets will provide the appropriate speed needed to get the spacecraft to go to
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Mars.
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The spacecraft consists of a cruise stage, which supply the communications and power
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during the seven-month journey to Mars, and a lander, which has the rover inside it.
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Upon arrival at Mars in January 2004, the landers are separated and enter the Martian
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atmosphere.
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Once the lander enters the Martian atmosphere, the aeroshell design will slow the entry from
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12,000 miles per hour to about 900 miles per hour.
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A parachute will then deploy, further slowing the spacecraft.
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Then airbags will inflate around the craft to cushion the landing.
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At about 600 feet above the surface, retro-rockets will fire, slowing the craft even further.
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Once the spacecraft stops rolling, the airbags will deflate and pedals will open up, bringing
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the lander to an upright position.
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Since the rovers carry all of their instruments on board, they'll be able to start exploring
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the planet almost immediately without having to stay close to the lander.
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How will the rovers be commanded?
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Will they be driven by remote control from Earth?
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Actually, the controllers from the Earth will only command the rovers to specific soil and
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rock targets.
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It'll be up to the rovers to find their own way to get there.
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The reason we have to do this is because a signal from Earth takes too long to get to
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Mars to have us operate them by remote control.
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As a result, the rovers must be able to operate autonomously.
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We will decide, based on information we get from the cameras and instruments that are
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sitting on the rover, where are good sites to go to and then command the rovers to go
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there.
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We hope the rovers will be able to travel up to a half a mile from the landing site.
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Okay, so once the rover gets to a rock of interest, how will it examine it?
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The rovers have many different instruments on there that allow us to examine the rocks
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down to the microscopic level.
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Once we analyze this type of information, we can tell a lot of different things about
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the rock themselves, like their mineralogy, elemental chemistry, their surface texture.
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This type of information will give us evidence of ancient environmental conditions and the
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possibility of some type of biological activity occurring.
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Recent satellite images of Mars show geologic features like channels, which support the
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theory that liquid water once flowed over the surface.
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Today, the Martian temperature is too low and the atmosphere too thin for liquid water
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to exist on the surface, but many scientists believe that liquid water may still exist
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below the surface of Mars where temperatures are not as harsh.
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If the rovers find convincing evidence of liquid water on Mars, then it's also possible
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they may find proof of life on Mars as well.
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There's a lot of evidence that there's frozen water just below the surface of Mars and a
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lot of these missions that we're trying to go to Mars in the next few years is trying
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to get a better understanding of how much water is there and is it in the liquid form
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near the surface somewhere.
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Three billion years ago, Mars and Earth were very much alike.
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Mars was, at that time, much wetter and much warmer than it is now and something has happened.
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So by trying to get a better understanding of how Mars' environment has evolved, it will
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give us a better understanding of potentially how the Earth's environment would evolve and
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give us an idea of how it's going to change in the future.
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So by studying Mars, it may be able to tell where our future is headed in this space?
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Exactly.
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The reason we are exploring Mars and other places in the solar system for that matter
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is to help answer two fundamental questions.
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One, to explain the formation and evolution of our solar system and the Earth within it
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and two, to seek the origins of life and its existence beyond the Earth.
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During the next decade, Mars will be the solar system's most popular travel destination.
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There are plans for nearly a dozen Mars missions being planned by three countries, the United
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States, Russia and Japan.
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Coming up, a new device developed by NASA might help parents and caregivers keep an
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electronic eye on their children.
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But first, did you know that the Viking 1 spacecraft was the first craft to land on
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the Martian surface on July 20, 1976?
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With its companion craft, Viking 2, the two landers analyzed atmospheric and weather conditions,
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collected soil samples and took over 56,000 pictures of the planet's surface.
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- Autor/es:
- NASA LaRC Office of Education
- Subido por:
- EducaMadrid
- Licencia:
- Reconocimiento - No comercial - Sin obra derivada
- Visualizaciones:
- 494
- Fecha:
- 28 de mayo de 2007 - 17:04
- Visibilidad:
- Público
- Enlace Relacionado:
- NASAs center for distance learning
- Duración:
- 06′ 25″
- Relación de aspecto:
- 4:3 Hasta 2009 fue el estándar utilizado en la televisión PAL; muchas pantallas de ordenador y televisores usan este estándar, erróneamente llamado cuadrado, cuando en la realidad es rectangular o wide.
- Resolución:
- 480x360 píxeles
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- 37.37 MBytes