AstroNews Sept 2002

Astronomy, space and ET news. http://www.kahl.net/astro

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AstroNews
Vol.4, No.9

NEXT GENERATION SPECIAL

  • EQUINOX
  • RARE LUNAR GLIMPSE
  • SKYWATCH 2003 IS OUT
  • SPACE CALENDAR
  • WHEEL WITHIN A WHEEL
  • NEXT GENERATION SPACE TELESCOPE
  • NEXT GENERATION PROPULSION
  • JAPAN'S NEXT GENERATION ROCKET

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Up This Month
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Look up!

EQUINOX
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Hey earthlings, happy EQUINOX!

Yessiree, it's that time of year when day and night are equally long. For us folks living on the northern half of our little blue planet, the 22nd of September signals the beginning of AUTUMN. And those of you "down under" are eagerly awaiting SPRING!

Equinox is when the Sun crosses the equator into southern skies. It will continue heading southward until the WINTER SOLSTICE in December, and will return to northern skies at the SPRING EQUINOX in March.

The FULL MOON closest to the autumnal equinox is known as the Harvest Moon, named so because the moonlight gave farmers extra time to harvest their crops.


RARE LUNAR GLIMPSE


In coming months early bird observers can spot the Moon’s most spectacular "hidden" landform. MARE ORIENTALE is a patch of dark lava flow on the western limb of the Moon. When this part of the lunar surface is in view, observers can glimpse its massive mountains projecting above the limb.

With the excellent October conditions you can see all the way across Mare Orientale to the Rook peaks jutting into space from the lunar farside.

Finding Orientale should be straightforward. Simply look along the limb just to the south of the well-defined dark patch of the crater Grimaldi. The long strips of dark lavas making up the two lakes will confirm your sighting of Orientale.

The best days are October 1st and 29th, November 25th, and December 22nd. A day before or after will still allow good views. With the Moon being so bright anyone even in a big city can try their luck at this!

Here's more from the Sky and Telescope website:
http://skyandtelescope.com/observing/objects/moon/article_723_1.asp

What else to keep your eyes peeled for? The Milky Way! It cuts the sky in half on autumn evenings. You'll need to be far away from city lights for a really spectacular view.

VENUS WAS HER NAME

And finally you must look out for VENUS playing the role of the evening star. It shines almost 20 times brighter than the brightest true star in the night sky. It's low in the southwest right after sunset, so you need a clear horizon.

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ASTROTIP


SKYWATCH 2003 IS OUT
~~~~~~~~~~~~~~~~~~~~
For a mere SIX DOLLARS you can order a thick magazine to keep you current for an entire year of skywatching. No need for a monthly subscription to an astronomy magazine if you aren't a card-carrying astronomy buff. Just grab a copy of SKYWATCH 2003 at your local newsstand.


SPACE CALENDAR

Thanks to new reader Karen for this link to an awesome Space Calendar that covers space-related activities and anniversaries for the coming year.

Compiled and maintained by Ron Baalke at Jet Propulsion Lab in Pasadena, CA (JPL), it includes over 1,100 links.

Space Calendar:
http://www.jpl.nasa.gov/calendar/


WHEEL WITHIN A WHEEL

Hubble Telescope photo of two spiral galaxiesThe name is rather plain: Hoag's Object. But imagine hot, blue stars in a sparkling ring around the core of a galaxy 60 million light years away in the constellation Serpens.

In 2001 Hubble Space Telescope took a gorgeous photo of this galactic pinwheel around a dense nucleus. It has recently been released and you can now admire in our AstroImage section!

The bright ring is filled with young stars, which are hotter and bluer than the older stars in the yellow core. The "gap" around the core may actually contain faint stars and star clusters. Even a small background galaxy appears just inside the ring at the upper right.

The galaxy is about 120,000 light-years across, slightly larger than our own Milky Way.

This galactic oddity exhibits no sign of a collision with a second galaxy. Some scientists theorize that the blue star circle is the remnant of a galaxy that passed close by the central one, some 2 billion or 3 billion years ago.

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DISTANT DISCOVERIES

NEXT GENERATION SPACE TELESCOPE

The successor to the Hubble Space Telescope is named the James Webb Space Telescope in honor of NASA's second administrator.

Hubble allowed us to see like no other telescope ever has. It shared with us the splendor of the cosmos, such as the birth and death of stars, the intricacies of other galaxies, and the universe as a toddler.

About eight years from now the James Webb Space Telescope will take over for Hubble. With a mirror more than twice the diameter of Hubble's, it will probe even farther into the universe and further back in time.

James E. Webb headed NASA from 1961 to 1968. During his tenure, NASA developed the Apollo program and launched more than 75 space science missions, including the first interplanetary explorers. Webb also believed that a major space telescope should be a priority for NASA.

TRW Inc. of Redondo Beach, California, will design and build the spacecraft and its 6-meter (20-foot) primary mirror for $825 million.

James Webb Space Telescope will travel to the L2 Lagrange point located 940,000 miles (1.5 million kilometers) from Earth, opposite the sun. This position will be gravitationally stable and allow the telescope to use a shield to block radiation from the sun, Earth, and the moon. This will also allow the spacecraft to remain cool without using a complex refrigeration system, but the telescope will also be too far away for shuttle astronauts to service the telescope as they do with Hubble.

With six times the light-gathering area as its predecessor, the new telescope will be able to view objects that are younger and nearer to the universe's birth than anything we've ever seen. But unlike Hubble, which observes in ultraviolet, visible, and near-infrared wavelengths, the James Webb Space Telescope will concentrate on the far visible to the mid-infrared range of the electromagnetic spectrum. It will be able to study the evolution of the first galaxies, probe disks around young stars for signs of forming planets, examine supermassive black holes, and make discoveries astronomers haven't yet imagined.

 

NEXT GENERATION PROPULSION

With space probes going ever farther conventional propulsion systems are proving way too inefficient. NASA has gone looking for more exotic ways to fly.

Chemical rockets are slow. They burn their propellant at the beginning of a flight and then the spacecraft just coasts the rest of the way. Although spacecraft can be sped up by gravity assist--a celestial crack-the-whip around planets, such as the one around Saturn that flung Voyager 1 to the edge of the solar system--round-trip travel times between planets are still measured in years and decades. A journey to the nearest star would take centuries if not millennia.

Chemical rockets are fuel-inefficient. Think of driving in a gas guzzler across a country with no gas stations. You'd have to carry boatloads of gas and not much else. In space missions, what you can carry on your trip that isn't fuel (or tanks for fuel) is called the payload mass--e.g., people, sensors, samplers, communications gear and food. Just as gas mileage is a useful figure of merit for the fuel efficiency of a car, the "payload mass fraction"--the ratio of a mission's payload mass to its total mass--is a useful figure of merit for the efficiency of propulsion systems.

With today's chemical rockets, payload mass fraction is low. Even using a minimum-energy trajectory to send a six-person crew from Earth to Mars, with chemical rockets alone the total launch mass would top 1,000 metric tons--of which some 90 percent would be fuel. The fuel alone would weigh twice as much as the completed International Space Station.

A single Mars expedition with today's chemical propulsion technology would require dozens of launches--most of which would simply be launching chemical fuel.

In other words, low-performance propulsion systems are one major reason why humans have not yet set foot on Mars.

More efficient propulsion systems increase the payload mass fraction by giving better "gas mileage" in space. Since you don't need as much propellant, you can carry more stuff, go in a smaller vehicle, and/or get there faster and cheaper. We need advanced propulsion technologies to enable a low-cost mission to Mars.

Thus, NASA is now developing ion drives, solar sails, and other exotic propulsion technologies using two basic approaches. The first is to develop radically new rockets that have an order-of-magnitude better fuel economy than chemical propulsion. The second is to develop "propellant-free" systems that are powered by resources abundant in the vacuum of deep space.

All these technologies share one key characteristic: They start slowly, They rely on the fact that a small continuous acceleration over months can ultimately propel a spacecraft far faster than one enormous initial kick followed by a long period of coasting.

They're all systems with low thrust but long operating times. After months of continuing small acceleration, you'd be clipping along at many miles per second. In contrast, chemical propulsion systems are high thrust and short operating times. After the initial lift off, the tank is empty.

Leading candidates for the advanced rocket are variants of ion engines. In current ion engines, the propellant is a colorless, tasteless, odorless inert gas, such as xenon. The gas fills a magnet-ringed chamber through which runs an electron beam. The electrons strike the gaseous atoms, knocking away an outer electron and turning neutral atoms into positively charged ions. Electrified grids with many holes (15,000 in today's versions) focus the ions toward the spaceship's exhaust. The ions shoot past the grids at speeds of up to more than 100,000 miles per hour (compare that to an Indianapolis 500 racecar at 225 mph)--accelerating out the engine into space, so producing thrust.

Where does the electricity come from to ionize the gas and charge the engine? Either from solar panels (solar electric propulsion) or from fission or fusion (nuclear electric propulsion). Solar electric propulsion engines would be most effective for robotic missions between the sun and Mars, and nuclear electric propulsion for robotic missions beyond Mars where sunlight is weak or for human missions where speed is of the essence.

Ion drives work. They've proven their mettle not only in tests on Earth, but in working spacecraft--the best-known being Deep Space 1, a small technology-testing mission powered by solar electric propulsion that flew by and took pictures of Comet Borrelly in September, 2001. Ion drives like the one that propelled Deep Space 1 are about 10 times as efficient as chemical rockets.

The lowest-mass propulsion systems, however, may be those that carry no on-board propellant at all. In fact, they're not even rockets. Instead, they relying on natural resources abundant in space for energy. The two leading candidates are solar sails and plasma sails. Although the effect is similar, the operating mechanisms are very different.

A solar sail consists of an enormous area of gossamer, highly reflective material that is unfurled in deep space to capture light from the sun (or from a microwave or laser beam from Earth). For very ambitious missions, sails could range up to many square kilometers in area.

Solar sails take advantage of the fact that solar photons, although having no mass, do have momentum--several micronewtons (about the weight of a coin) per square meter at the distance of Earth. This gentle radiation pressure will slowly but surely accelerate the sail and its payload away from the sun, reaching speeds of up to 150,000 miles per hour, or more than 40 miles per second.

A common misconception is that solar sails catch the solar wind, a stream of energetic electrons and protons that boil away from the Sun's outer atmosphere. Not so. Solar sails get their momentum from sunlight itself. It is possible, however, to tap the momentum of the solar wind using plasma sails.

Plasma sails are modeled on Earth's own magnetic field. Powerful on-board electromagnets would surround a spacecraft with a magnetic bubble 15 or 20 kilometers across. High-speed charged particles in the solar wind would push the magnetic bubble, just as they do Earth's magnetic field. Earth doesn't move when it's pushed in this way--the planet is too massive. But a spacecraft would be gradually shoved away from the Sun.

Of course, the original, tried-and-true propellant-free technology is gravity assist. When a spacecraft swings by a planet, it can steal some of the planet's orbital momentum. This hardly makes a difference to a massive planet, but it can impressively boost the velocity of a spacecraft. For example, when Galileo swung by Earth in 1990, the speed of the spacecraft increased by 11,620 mph; meanwhile Earth slowed down in its orbit by an amount less than 5 billionths of an inch per year. Such gravity assists are valuable in supplementing any form of propulsion system.

Slowing down and stopped presents another problem for propulsion systems. With chemical propulsion, the usual technique is to fire retrorockets--once again, requiring large masses of onboard fuel.

A far more economical option is promised by aerocapture--braking the spacecraft by friction with the destination planet's own atmosphere. The trick, of course, is not to let a high-speed interplanetary spacecraft burn up. But NASA scientists say, with an appropriately designed heat shield, it would be possible for many missions to be captured into orbit around a destination planet with just one pass through its upper atmosphere.

A hybrid of several technologies could prove to be very economical in getting a manned mission to Mars. In fact, a combination of chemical propulsion, ion propulsion, and aerocapture could reduce the launch mass of a six-person Mars mission to below 450 metric tons (requiring only six launches)--less than half that attainable with chemical propulsion alone.

Such a hybrid mission might go like this: Chemical rockets, as usual, would get the spacecraft off the ground. Once in low-Earth orbit, ion drive modules would ignite, or ground controllers might deploy a solar or plasma sail. For 6 to 12 months, the spaceship--temporarily unmanned to avoid exposing the crew to large doses of radiation in Earth's Van Allen radiation belts--would spiral away, gradually accelerating up to a final high Earth-departure orbit. The crew would then be ferried out to the Mars vehicle in a high-speed taxi; a small chemical stage would then kick the vehicle up to escape velocity, and it would head onward to Mars.

As Earth and Mars revolve in their respective orbits, the relative geometry between the two planets is constantly changing. Although launch opportunities to Mars occur every 26 months, the optimal alignments for the cheapest, fastest possible trips happen every 15 years--the next one coming in 2018.

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FAR OUT FACTS

JAPAN'S NEXT GENERATION ROCKET

Japan's new-generation space rocket deployed satellites for the first time, marking what officials said was a major step towards a commercial satellite launch business.

The 57-meter (190-foot) H-2A rocket, carrying two satellites -- a data relay satellite and an unmanned space experiment recovery system -- blasted off from Tanegashima, about 1,000 km (625 miles) southwest of Tokyo, at 5:20 p.m. (0820 GMT) on Tuesday.

"Today's launch marks a major step towards commercialization of Japan's satellite launch business," said an official of the National Space Development Agency (NASDA).

Japan launched its first H-2A rocket, without a payload, in August 2001, but when it launched its second last February it failed to put a test satellite into orbit.

The smooth launch of the latest version of the home-grown rocket had been seen as crucial to the future of Japan's fledgling space program, which critics have slammed for its expense and a series of launch failures.

The cost of manufacturing the rocket and launching it was 10.2 billion yen ($85.76 million), the NASDA official said.

The data relay satellite cost 31.8 billion yen and the space experiment recovery system about 20 billion.

A mishap in 1999 resulted in the loss of a 10 billion yen prototype, while another unsuccessful launch the year before cost 60 billion yen.
Competitive market

H-2A rockets are intended for commercial use in the global market, which is dominated by European Ariane rockets, followed by U.S., Chinese and Russian space launches.

Japan, plagued by the humiliating mishaps, has struggled to secure international trust in its launch capabilities.

In May 2000, U.S. satellite maker Hughes Space and Communications, which had agreed to use Japanese rockets to launch 10 satellites, terminated the contracts because it had lost confidence in Japan's space technology.

The Japanese government plans to privatize the H-2A rocket business in 2005.

The Science and Technology Ministry was expected to decide in November to hand over the manufacturing technology of the H-2A rockets to Mitsubishi Heavy Industries Ltd (MHI), government sources have said.

The transfer of the H-2A manufacturing technology to MHI from NASDA will pave the way for MHI to expand into the aerospace business, including rocket manufacturing and satellite launches.

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