Owen, spectacled and goofy as the stereotypical math geek, suits the film's taste for typecasting as well as its quaintly 1950's look, which calls for studiously modest props and costumes and for townsfolk who are often Rockwellishly agog. But he brings such sincerity to telling his science teacher that a book called ''Principles of Guided Missile Design'' is the best present he has ever received that his affecting performance is liable to breathe life into science projects everywhere. Gyllenhaal does seem more like the Columbia University freshman he is than the rural West Virginian he plays. And a pretty girl is on hand to sigh, ''It sure was exciting watching your rockets go up!'' In a film that appreciates the advent of ''Jailhouse Rock'' along with that of Sputnik, ''Ain't That a Shame?'' accompanies a montage of rockets gone kerflooey. Since this means commandeering metal from railroad tracks and visiting a still for 100-proof rocket fuel, the story has its playful side. With the aid of his closest buddies (Chris Owen, William Lee Scott and Chad Lindberg), Homer draws on limited local resources for his rocketry experiments.
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The film watches Homer progress from accidentally blowing a hole in the family's white picket fence, which virtually adjoins the mine, to learning how to make a rocket soar. And Homer, played with beguiling eagerness by Jake Gyllenhaal, has to choose between frustrating his father and shooting for the stars.
The senior Hickam, played by Chris Cooper as a headstrong man to be reckoned with, is a hard-driving mine foreman who simply has no way of understanding his son's aspirations. And it makes the tension between this teen-ager and his tough coal-mining father its main concern. Hickam's folksy, best-selling memoir, ''Rocket Boys,'' Joe Johnston's second and better rocket film (after ''The Rocketeer'') contrasts Homer's high hopes with his all-but-certain destiny. The difference between aiming sky high or descending into the mine is heavily emphasized, in both visual and dramatic terms.īased on Mr. grew up in a West Virginia coal mining town and went from telling schoolmates, ''I'm gonna build a rocket like Sputnik!'' to a career as a NASA engineer. With the gung-ho wholesomeness of a Horatio Alger story by way of Norman Rockwell, it tells how Homer H. Otherwise, despite its ''based on a true story'' opening credit, this earnest, nostalgic film has a way of seeming too good to be true. This process is experimental and the keywords may be updated as the learning algorithm improves.By far the most moving scenes in ''October Sky'' are the home-movie snippets, circa 1957, that show the real people on whom the film's characters are based. These keywords were added by machine and not by the authors. These latter sources are supposed to be stars with dust envelopes Keywords Half of them are well described by a black body spectrum, while the others show a flat or redder spectrum.
Sixty-two of 680 IRAS sources in the region spatially coincide with the detected sources and the spectrum energy distributions from 1.25μm to 100μm were derived for these 62 sources. The detected sources are cross-identified with the IRAS Point Source Catalog. This supports the idea that the position of the active star forming region has changed during the past 10 8 years. The distributions of RSG, luminous giants and CO line flux are spatially different from each other. The dominant components of the sources are red super giants (RSG), luminous M-type giants and AGB stars in the LMC. The positions and the J, H, and K’ magnitudes were derived for 1599 point sources whose S/N ratio were more than four at the K’-band. The limiting magnitudes of the survey were 13.6, 11.9, and 10.0 magnitude (3σ) at the J, H, and K’ bands, respectively. The system was attached onto the Automated Patrol Telescope of the University of New South Wales. The plate scale was 4.″6 x 6.″0/pixel and the total field of view was 40.′2 x 52.′3. We used a 25 cm/F3.5 Newtonian telescope equipped with a 512x512 PtSi-Camera (Ueno et al. The observations were performed from Oct to Nov, 1994 at the Siding Spring Observatory. We surveyed the central 3° x 6° region of the Large Magellanic Cloud (LMC) with angular resolution of 10″.0 at the J(1.25μm), H(1.65μm) and K′(2.15μm) bands.
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