Sunday, January 4, 2015

A Close Encounter With Poor Pluto!

There is a cold, dimly lit, and mysterious region far beyond the beautiful blue ice-giant Neptune--the most distant of the eight major planets from our Sun. In this faraway domain called the Kuiper belt--that astronomers are only now beginning to explore--a myriad of strange, icy worldlets dance around our Star. Pluto, one of the largest worlds inhabiting the Kuiper belt, was originally classified as the ninth major planet from the Sun after its discovery in 1930, but the realization that this icy little oddball is only one of several large frozen bodies dwelling in the Kuiper belt prompted the International Astronomical Union (IAU) to formally define "planet" in 2006--and poor Pluto was unceremoniously booted out of the pantheon of major planets. Pluto, now newly reclassified as a mere dwarf planet is nonetheless an object of considerable interest, debate, and affection. Soon scientists will know much more about this beloved little ice ball far, far away because, after a journey of almost nine years and three billion miles--the farthest any space mission has ever traveled to reach its main target--NASA's New Horizons spacecraft came out of hibernation on December 6, 2014 in preparation for its long-awaited 2015 close encounter with Pluto.
Mission scientists at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Maryland, confirmed on December 6, 2014 that New Horizons, operating on pre-programmed computer commands, had successfully switched from its hibernation mode to its "active" mode. Zipping along at the breathtaking speed of light, the radio signal dispatched from New Horizons--which, as of this writing, has journeyed over 2.9 billion miles from Earth, and just over 162 million miles from Pluto--required four hours and 26 minutes to reach NASA's Deep Space Network Station located in Canberra, Australia.
"This is a watershed event that signals the end of New Horizons crossing of a vast ocean of space to the very frontier of our Solar System, and the beginning of the mission's primary objective: the exploration of Pluto and its many moons in 2015," explained Dr. Alan Stern in a December 6, 2014 APL Press Release. Dr. Stern, who is from the Southwest Research Institute in Boulder, Colorado, is New Horizons Principal Investigator.
Since its launch on January 19, 2006, New Horizons has spent 1,873 days--or about two-thirds of its flight time--in hibernation mode. Its 18 separate hibernation periods, from mid-2007 to late 2014, ranged from 36 days to 202 days in duration. The science team used hibernation mode to save wear and tear on the long-journeying spacecraft components and lessen the risk of system failures.
"Technically, this was routine, since the wake-up was a procedure that we'd done many times before. Symbolically, however, this is a big deal. It means the start of our pre-encounter operations," explained Dr. Glen Fountain in the December 6, 2014 APL Press Release. Dr. Fountain is New Horizons Project Manager at APL.

Alas, Poor Pluto!
Pluto is a relatively large inhabitant of the frigid, dark Kuiper belt, where it circles around our Sun in the enchanting company of a vast multitude of mysterious, bewitching icy objects of its own kind. From this very distant domain, our Sun appears as only an especially large star suspended in the dark sky!
Like other Kuiper Belt Objects (KBOs), Pluto is thought to be primarily made up of rock and ice. It is a relatively small world, only about 1/6 the mass of Earth's Moon and 1/3 its volume. Pluto also sports an eccentric and highly inclined orbit that takes it from 30 to 49 Astronomical Units (AU) from our Star. One AU is equivalent to the average Earth-Sun separation, which is 93,000,000 miles. Therefore, Pluto periodically approaches our Sun at a distance closer than Neptune! However, an orbital resonance with Neptune very fortunately prevents the two worlds from blasting into each other.
The Kuiper belt, sometimes called the Edgeworth-Kuiper Belt, is a distant region of our Solar System beyond the realm of the planets. It extends from the orbit of Neptune to approximately 50 AU. Neptune's average distance from our Star is 30.1 AU--it's perihelion (closest to our Sun) is 29.8 AU, while its aphelion (most distant from our Sun) is 30.4 AU.
The demoted icy oddball that is Pluto was discovered by the American astronomer Clyde Tombaugh in 1930, and this small world, shrouded in perpetual darkness where it dwells in the deep freeze of our Solar System's outer limits, was appropriately named in honor of the Roman god of the underworld. Pluto's largest moon, Charon, was discovered in 1978 by astronomer James Christy, also an American. Charon is thought to be a chunk torn off from Pluto itself during a catastrophic collision between Pluto and some other object that was also tumbling around close to it in the Kuiper belt.
For most of the 20th century, it was wrongly believed that Pluto is a solitary little world where it dwells in the frigid darkness, far from the comforting light and warmth of our Star. However, in 1992, the very first KBO was discovered, and astronomers soon realized that Pluto is not far from the madding crowd of a multitude of other KBOs. Indeed, since then, many other small icy worldlets akin to Pluto--also sporting eccentric orbits--have been spotted. The most notable of these is the scattered disc object dubbed Eris, that was discovered in 2005. Eris is approximately 27% more massive than Pluto. The understanding that Pluto is merely one of many resulted in its demotion and reclassification. However, there are astronomers who oppose this demotion, arguing that Pluto should have retained its classification as a major planet, and that the other kindred dwarf planets that have been discovered should be added to the list of major planets along with Pluto.
Pluto itself has five known moons: Charon, Nix, Hydra, Kerberos, and Styx. Charon is by far the largest of Pluto's moons, and it boasts a diameter of approximately 50% that of Pluto. Some astronomers consider Pluto and Charon to be a binary system because the barycenter of their orbits does not lie within either world. However, as of this writing, the IAU has yet to provide a definition for binary dwarf planets. Because of this, Charon is still officially classified as a moon of the dwarf planet Pluto.
Pluto has a very thin atmosphere composed of nitrogen, methane, and extremely toxic carbon monoxide, which is probably derived from the ice on Pluto's frozen surface. As Pluto makes its way ever closer to our Star in its orbit it grows warmer and warmer. The ice on its surface evaporates as a result, and the gasses slowly float away into interplanetary space. This continues until Pluto starts to make its long journey away from the Sun again, becoming colder and colder as it does so. Pluto's atmosphere again freezes, and then falls down to its surface as snow--but it will evaporate again when Pluto begins its long journey towards our Sun. Pluto's last approach to our Star was back in 1989. It takes 248 years for the frozen little world to finish only a single orbit around our Sun.

A Close Encounter With Poor Pluto!
The "active" mode awakening New Horizons from its hibernation was programmed into the spacecraft's onboard computer in August 2014, and it started to work aboard New Horizons on December 6, 2014. About one hour and a half after starting, New Horizons began transmitting signals to Earth reporting on its condition--including the news that it was back in "active" mode.
The New Horizons team plans to spend several weeks monitoring the spacecraft, making certain that its systems and science instruments are performing as they should. The scientists will also continue to build and test the computer-command sequences that will take New Horizons through its journey to, and close encounter with, the Pluto system.
Carrying a seven-instrument science payload, including sophisticated imaging infrared and ultraviolet spectrometers, two powerful particle spectrometers, a space-dust detector, and a compact multicolor camera, New Horizons is scheduled to begin its mission of observing the mysterious Pluto system on January 15, 2015.
New Horizons closest approach to its quarry will occur on July 14, 2015, but a treasure trove of new discoveries are expected to be made before then--including, by mid-May 2015, views of the Pluto system that are far superior to what even the venerable Hubble Space Telescope is able to provide of this bewitching little ice-world and its many frozen moons.
"New Horizons is on a journey to a new class of planets we've never seen, in a place we've never been before. For decades we thought Pluto was this odd little body on the planetary outskirts; now we know it's really a gateway to an entire region of new worlds in the Kuiper belt, and New Horizons is going to provide the first close-up look at them," New Horizons Project Scientist Dr. Hal Weaver, of APL, told the press on December 6, 2014.
Judith E. Braffman-Miller is a writer and astronomer whose articles have been published since 1981 in various newspapers, journals, and magazines. Although she has written on a variety of topics, she particularly loves writing about astronomy because it gives her the opportunity to communicate to others the many wonders of her field. Her first book, "Wisps, Ashes, and Smoke," will be published soon.

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