RocketSTEM Issue #10 - February 2015 | Page 58

discover the comet’s surface was group of 11 different science instruOn Oct. 18, 2004, ESA gave the not as expected. When viewed in ments aboard Rosetta, all designed green light for Philae to attempt the the ultraviolet portion of the specto help unlock the secrets of comet first-ever soft landing on the surface trum, they observed the surface to 67P. NASA is also contributing to the of a comet. After weeks of scrutinizbe darker than charcoal and void Microwave Instrument for Rosetta ing images and date from Rosetta, of any large, icy patches. Due to its Orbiter (MIRO), the Ion and Electron the team selected site J, located location and distance from on the head of the comet, the Sun, any exposed waas the primary landing site. ter-ice would not be vaporFollowing a public conized by the Sun and would test, the site was dubbed be present on the surface. Agilkia, in honor of an island located on the Nile river. Alan Stern, ALICE prinAgilkia is located close to cipal investigator at the the site where the Philae Southwest Institute in obelisk was discovered. Boulder, Colorado stated: “We’re a bit surprised at At 3:35 a.m. EST (0835 just how unreflective the GMT) on Nov. 12, Rosetta comet’s surface is and released Philae, to start its how little evidence of exseven-hour free-fall to the posed water-ice it shows.” comet’s surface. The landing process is a fully auALICE also detected the tonomous process, with ESA presence of both hydrogen supplying instructions to the Comparing Comet 67P/Churyumov–Gerasimenko with the city of Paris. and oxygen in the comet’s Credit: ESA/Rosetta/Navcam/Google/Bluesky spacecraft and the lander coma (atmosphere). prior to release. It takes The ALICE instrument is Sensor (IES), a portion of the Rosetta 28-minutes for the signal from Rosetta packed with over 1,000 times the Plasma Consortium Suite, and the to reach us here on Earth, so ESA data-gathering capabilities of the Double Focusing Mass Spectromexpected to receive landing confirprevious generation’s instruments, eter (DFMS) electronics package for mation at 11:00 a.m. EST (1600 GMT). while weighing under nine pounds the Rosetta Orbiter Spectrometer (4 kilograms) and drawing only 4 Forty-five years ago, the world for Ion Neutral Analysis (ROSINA). watts of power. ALICE is part of a waited, glued to their television sets Astronomical serendipity Since 1594, when Johannes Kepler predicted that there should be a planet between Mars and Jupiter, astronomers had been searching for that “missing planet.” When Giuseppe Piazzi discovered Ceres in 1801, the scientific world thought that he had ended the search. Then Ceres disappeared from sight, only to be recovered one year later. Astronomers breathed a sigh of relief and celebrated! The “missing planet” was back! And then there were two Wilhelm Olbers, an amateur German astronomer who was a doctor by profession, was again looking for Ceres about three months after it had been rediscovered. That was when he saw another moving object nearby! This “object,”, which was later named Pallas, caused quite a stir in the astronomical community. Only one planet had been expected in the space between Mars and Jupiter. When Gauss calculated this new object’s orbit, he found that both Ceres and Pallas took 4.6 years to revolve around the sun. He also found that Pallas could be seen from the Earth for only a small portion of that time. It was incredible luck and timing or, 56 56 maybe astronomical serendipity that Olbers was looking for Ceres during the short period of time that Pallas happened to be passing near Ceres. Otherwise,