Why launch Chandra at night?
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Blame Newton and Kepler
by tides and radiation belts
July 23, 1999: Why launch in the middle of the night? Blame Johannes Kepler and Isaac Newton and the engineers who designed the Chandra X-ray Observatory.
It starts in orbital mechanics, a sometimes obscure but always essential part of space travel. The field is rooted in the earliest days of modern astronomy, when Kepler discovered that planets moved in well-regulated elliptical paths and Newton discovered that gravity is universal. Newton also invented the calculus that became the foundation of the complex math used in planning satellite orbits.
But we can't always use it to avoid working late at night.
Chandra's night launch time was set by several factors, starting with the need to protect the telescope's science instruments from damage in the Van Allen Radiation Belts.
To avoid most of the belts, Chandra would have to be placed in a highly elliptical orbit. That makes tidal forces a bigger concern than they would be for a satellite in low Earth orbit, explained Dr. Jonathan McDowell, a scientist with the Chandra Science Center in Cambridge, Mass.
"It was not picked for any astronomical reason. It was picked for orbital lifetime as determined by lunar and solar perturbations," he said. Highly eccentric orbits will have their perigee (point closest to the Earth) shifted up and down by tidal forces from the Sun and Moon. "The trick is to choose an orbital plane where you ensure a long orbit."
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Chandra's orbit has a period of 64.2 hours, with about 15 hours of that inside the Van Allen Radiation Belts, forcing operators to shut down the science instruments while the observatory is below 60,000 km (24,000 mi) altitude. Essential chores like repointing the observatory and moving gratings into and out of the light path that would disrupt science observations will be scheduled for the passes through the radiation belts.
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Large orbits are nearly fixed in inertial space. Just as the Earth and the rest of the planets have orbits that keep virtually the same orientation relative to the galaxy, with only gradual changes over long periods, Chandra's orbit will hold the same orientation.
That also means that when Chandra is near apogee, the Earth will always be in the same section of Chandra's sky. Because Chandra can't look within 20 deg. of the Earth (an angle about 40 times larger than the size of the Moon as we see it from Earth), the same small chunk of sky will be largely off limits for a long time.
"It's part of the price you pay for being in a deep orbit," McDowell said.
The obscured zone covers an area from 4 to 11 hours right ascension and -10 to -50 deg. declination, roughly opposite the galactic center. It's not a total blackout, just a sharp enough reduction in observing time in that area that little science of value would be achieved.
Fortunately, McDowell noted, that part of the sky has a few choice targets. McDowell noted that planners for Europe's Infrared Space Observatory actually did have a choice, a tough one, when they opted for an eccentric orbit. They had to give up the galactic center or the Orion nebula, both areas of remarkable activity in infrared light. They chose the galactic center, but ISO lasted long enough for its orbit to shift and let them view Orion.
How does all this lead to a launch at around midnight?
Simple. Imagine Chandra's final orbit as an ellipse moving with the Earth around the Sun. Even as the Earth spins, the ellipse stays pointed in the same direction. Launch and all the intermediate steps to get to the final orbit all lie within this ellipse.
An additional factor, McDowell explained, is that Chandra has strict power requirements, so it must be oriented to expose its solar arrays properly during maneuvers to its final orbit. Furthermore, the upper stages have a horizon sensor that must look in a certain direction. These two bits of spacecraft geometry are what finally set Chandra's launch time relative to the stars, not human work schedules.
For a launch on July 20, 1999, Kennedy Space Center rotated into position on the ellipse's plane at 12:36 a.m. EDT. For every day of delay, McDowell noted, Chandra's launch moves up by 4 minutes. If Chandra was launched around Jan. 20, launch would be in the afternoon 12:36 p.m.
| Web Links |
| Xrayastronomy.com, science news from the Chandra X-Ray Observatory STS-93, the Chandra mission, launch status at Kennedy Space Center. Chandra X-ray Observatory Center home page, with links to education, news, and technical pages. Chandra news from Marshall Space Flight Center Chandra Project Science is managed at NASA/Marshall, has links to individual instruments and the prime contractor. X-ray astrophysics branch at NASA/Marshall conducts a broad range of research and technology work, as well as supporting the Chandra X-ray Observatory. NASA/Marshall scientists will use Chandra to study: Pulsars in the Fast Lane - Scientists are looking for bizarre, short-lived, powerhouse stars that burst with some of the brightest energy in the universe. Why did the supernova change colors? - SN 1993J was seen to be one kind of massive explosion, but then seemed to morph into a distinctly different kind. How hot is the Crab? - NASA's next Great Observatory takes aim at the Crab Nebula pulsar. Chandra will target the age of the Universe - Astronomers plan to combine radio images of galaxy clusters with new data from the Chandra X-ray Observatory and open a new window on the history of the Universe. |
Right: Engineers from NASA/Marshall wait for launch. NASA photo.
Even so, the blocked area eventually will become available. The same forces that make tides rise and fall will slowly shift Chandra's orbit, so that the blocked area is clear after a few years - but at the expense of blocking something else.
Those forces will also bring Chandra home. McDowell said that after the perigee is shifted higher by solar perturbations, it will be shifted lower so that by 2029, give or take a few years - and long after it has ceased operations - Chandra will become a shooting star blazing through Earth's atmosphere.
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| For more information, please contact: Dr. John M. Horack , Director of Science Communications |
Author: Dave Dooling Curator: Linda Porter NASA Official: M. Frank Rose |
