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Getting There

launchvehicle

 

We are going...

NASA reserachers and engineers cannot identify all that we will gain from space exploration in the future; however, the return on our investment will be great because the Vision for Space Exploration states as one of the goals: "...to advance U.S. scientific, security, and economic interests through a robust space exploration program." 

In the past, NASA's human space flight and robotic exploration programs have largely oeprated independently of each other.  However, this is quickly changing.  Coordination and integration will be an essential part of the future of exploration.

Over the next three decades, NASA will send robotic missions to the Moon, Mars, the moons of Jupiter, and other planetary bodies in the outer solar system.  These robots will serve as counterparts to human explorers by going where humans cannot go providing an extra set of "hands and eyes".  These robotic explorers will visit new worlds to obtain scientific data, demnonstrate technology capabilities, identify space resources, and gather critical information to maintaining health and productivity of human explorers.  They will also serve as testbeds for developing and testing technologies that will eventually carry human explorers beyond low Earth orbit.

When do we go?

The distance between Mars and Earth varies because, like all planets, they have elliptical (oval) orbits. Earth's orbit is only slightly elliptical; Mars's orbit is more so. Each planet also takes a different amount of time to travel round its orbit: 365 days for Earth and 687 Earth-days for Mars. Think of the two planets as bicycles racing on a track. Earth is traveling faster than Mars on the inside track, so it will periodically catch up and overtake it. When Earth is on the point of overtaking Mars, the two planets are lined up with the Sun. Click here for an interactive shockwave simulation showing the two orbits.

When the planets are lined up, it is called an opposition because, as seen from Earth, Mars is opposite the Sun in the sky. Mars oppositions occur approximately once every 780 days (or about 2 Earth years). These are optimal times to travel to Mars because the planets are closer together. They are also good times to view Mars from the Earth because all of Mars illuminated side faces us.

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Mars 2003 perihelion opposition

Click to enlarge.

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Mars 2010 aphelion opposition

Click to enlarge.

If opposition occurs when Mars is at its closest proximity to the Sun (a position on its elliptical orbit called perihelion), the distance between the two planets will be a minimum – about 55 million kilometers. When Mars is at its farthest point from the Sun (called aphelion), the distance at opposition will be about 99 million kilometers. A spacecraft to Mars can be launched around any opposition, about once every 26 months, but the journey will be shortest and use the least fuel around a perihelic opposition, which occurs about once every 17 years. The next time this will happen is 2020. 

How do we go?

We use rockets or launch vehicles to boost robotic spacecraft into orbit around the Earth. The spacecraft then uses its own rocket engine to lift it out of Earth orbit and to send it on its way to Mars. This is called the trans-Mars injection burn or TMI. Current robotic spacecraft use chemical fuels for propulsion and solar or nuclear power for electrical energy. Radio communications between the spacecraft computer and computers on Earth help to track and guide the spacecraft.

So far the U.S. has only sent spacecraft on one-way journeys into the solar system. The Stardust mission to a comet includes a sample return spacecraft.  The projected Mars Sample Return missions would also bring spacecraft (and samples) back to Earth.

How long does it take?

Spacecraft traveling through the solar system start out at relatively fast speeds (if they are moving away from the Sun) and slow down during flight. As they begin to enter into the gravitational pull of the target body, they begin to speed up again. Course corrections during the mission generally do not affect overall travel speeds. Many missions to the outer planets use the slingshot approach to help speed up.  This means they use the gravitational force of a passing planet to pull them past and around and send them off at higher speeds. Trips to the planet Mars would not use this method, however. The travel times of the missions that have been sent to Mars have varied slightly depending on where the Earth and Mars are in their respective orbits. Most missions have taken spacecraft from six to twelve months to reach Mars.

What are the risks?

All space missions, including those without humans on board, entail a variety of risks. There are risks to the spacecraft systems caused by external forces and internal mechanisms. Spacecraft can be affected by cosmic and solar radiation, micrometeorite and meteorite damage, and a vast array of problems connected to the complexity of the engineering designs and requirements of the spacecraft itself. Robotic spacecraft, which are extremely complex, are composed of many delicate systems including propulsion, communications, guidance and payload (the experiments and instruments onboard the spacecraft). Humans, who are not without fault, design these spacecraft and errors do occur. NASA has a policy of redundancy that requires backup systems for all mechanical functions on a spacecraft. This can help ensure the success of the mission.

Questions to think about:

  • If you were planning a series of missions to Mars, how would you go about planning your timeline?
  • In planning missions to other planets, how can you justify the importance of exploration versus the high cost of sending missions that might fail?
  • What kinds of measures can you take to help ensure spacecraft safety and success?

Next... Mariner Missions (pg. 3 of 12)


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