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originally posted by: Sammamishman
a reply to: Krakatoa
How about "Laira"? ....too obscure?
originally posted by: jhn7537
Hey ATS... This thread will be short and sweet. A girl I know who lives in the Houston area just posted this photo asking if anyone else saw this tonight?
I'm assuming meteor entering the atmosphere? I'm no expert on these type of things, but I figured I'd run it by ATS..
originally posted by: Sammamishman
Looks to be a meteor or space debris on both accounts. If it seems to break-up, come apart, shoot sparks off or vary wildly in brightness and color as it comes into view and then disappears, it tends to scream meteor.
If it stays a fairly constant brightness and color across it entire visible flight path then I would sit up and take notice.
A meteors make up makes it almost impossible to not spark or lose peices of itself coming through the air.
originally posted by: Sammamishman
A meteors make up makes it almost impossible to not spark or lose peices of itself coming through the air.
Depending on it's size, a dense iron/nickel meteoroid can stay intact enough as it burns up in the atmosphere to not have any visual sparks or anything breaking off. Chondrites, achondrites and stony-iron meteoroids however put on a show when they burn-up, break-up and spark as long as they are large enough to be visible far a long enough period of time.
Vivid colors are more often reported by fireball observers because the brightness is great enough to fall well within the range of human color vision. These must be treated with some caution, however, because of well-known effects associated with the persistence of vision. Reported colors range across the spectrum, from red to bright blue, and (rarely) violet. The dominant composition of a meteoroid can play an important part in the observed colors of a fireball, with certain elements displaying signature colors when vaporized. For example, sodium produces a bright yellow color, nickel shows as green, and magnesium as blue-white. The velocity of the meteor also plays an important role, since a higher level of kinetic energy will intensify certain colors compared to others. Among fainter objects, it seems to be reported that slow meteors are red or orange, while fast meteors frequently have a blue color, but for fireballs the situation seems more complex than that, but perhaps only because of the curiosities of color vision as mentioned above.
The difficulties of specifying meteor color arise because meteor light is dominated by an emission, rather than a continuous, spectrum. The majority of light from a fireball radiates from a compact cloud of material immediately surrounding the meteoroid or closely trailing it. 95% of this cloud consists of atoms from the surrounding atmosphere; the balance consists of atoms of vaporized elements from the meteoroid itself. These excited particles will emit light at wavelengths characteristic for each element. The most common emission lines observed in the visual portion of the spectrum from ablated material in the fireball head originate from iron (Fe), magnesium (Mg), and sodium (Na). Silicon (Si) may be under-represented due to incomplete dissociation of SiO2 molecules. Manganese (Mn), Chromium (Cr), Copper (Cu) have been observed in fireball spectra, along with rarer elements. The refractory elements Aluminum (Al), Calcium (Ca), and Titanium (Ti) tend to be incompletely vaporized and thus also under-represented in fireball spectra.