Though they are real stars – not just some fictional
astronomical phenomena conjured up in Gene Roddenberry’s Star Trek – are Y-Class
brown dwarf stars truly qualify as the coolest stars ever in terms of
temperature?
By: Ringo Bones
Given that a star’s spectral class / color temperature can now
easily determined after seeing it and taking spectroscopic , bolometric and
other tests via that “Oh Be A Fine Girl Kiss Me Smack” mnemonic device. But it
seems we still have to add another letter to than mnemonic device to accommodate
recently discovered new classes of stars that – if you were to excuse the pun –
are actually very cool. The latest stellar spectral type classification mnemonic
had to be changed and now goes as: “Oh Be A Fine Girl Kiss Me Less Tongue, Yo”.
Discovered back in 2011 by the onboard astronomical instruments
on the Wide-field Infrared Survey Explorer or WISE spacecraft that “see” in the
infrared portion of the electromagnetic spectrum, Y Class Brown Dwarf stars
were said to be the coolest stars discovered to date. Despite the existence of
clouds of iron vapor being picked up by the WISE spacecraft’s instrument and “snow”
made up of iron filings on a Y-Class Brown Dwarf star it is studying, the mean
surface temperature of the said star is only 80 degrees Fahrenheit - a temperature cool enough to be touched with
one’s own hands.
Basing on the data gathered so far astronomers believe that
Y-Class Brown Dwarf stars are believed to be an intermediate stage between
planets and stars. They are on average bigger than the planet Jupiter. While
some astronomers label them as “failed stars” – as in stars not big enough to
have the requisite gravity to initiate full blown fusion to burn hot enough to
be a bona-fide star.
2 comments:
Y-Class Brown Dwarf Stars could me Mother Nature's version of that 13 year-old UK student Jamie Edward's school science project mini fusion power plant or proof that cold fusion is more than just an alternative energy crank.
For Star Trek fans curious about Y-Class Brown Dwarf Stars, in the Star Trek: The Next Generation second season episode titled Manhunt, Commander Data mentioned about the differences in the europium-gadolinium-samarium ratios between ordinary stars and Y-Class Brown Dwarf Stars in an after-dinner conversation between Captain Picard and Lwaxana Troi.
Post a Comment