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Galaxies come in three main types: elliptical, spirals, and irregulars. A slightly more extensive description of galaxy types based on their look is given by the Hubble sequence. Since the Hubble sequence is completely based upon visual morphological type, it may miss certain significant individuality of galaxies such as star formation rate or activity in the core.

Our own galaxy, the Milky Way, occasionally simply called the Galaxy (with uppercase), is a large disk-shaped barred spiral galaxy about 30 kilo parsecs or a hundred light millennia in diameter and three light millennia in thickness. It contains about 3×1011 (three hundred billion) stars and has a whole mass of about 6×1011 (six hundred billion) times the mass of Sol.

In spiral galaxies, the spiral arms have the contour of approximate logarithmic spirals, a pattern that can be notionally shown to result from a disturbance in a uniformly rotating mass of stars. Like the stars, the spiral arms also revolve around the center, but they do so with steady angular velocity. That means that stars pass in and out of spiral arms. The spiral arms are consideration to be areas of high density or density waves. As stars move into an arm, they slow down, thus creating a higher density; this is akin to a "wave" of slowdowns moving along a highway full of moving cars. The arms are noticeable because the high density facilitates star formation and they therefore port many bright and young stars.

Despite the fame of large elliptical and spiral galaxies, most galaxies in the universe appear to be dwarf galaxies. These tiny galaxies are about one hundred times smaller than the Milky Way, holding only a few billion stars. Many dwarf galaxies may orbit a single larger galaxy; the Milky Way has at least a dozen such satellites. Dwarf galaxies may also be classified as elliptical, spiral or uneven. Since small dwarf ellipticals bear little resemblance to large ellipticals, they are often called dwarf spheroidal galaxies instead.

Boxing, as well called pugilism, Western Boxing, prizefighting, when referring to specialized boxing, or a widespread nickname among fans, is a sport in which two contributors of similar weight fight each other with their fists in a series of one to three-minute gaps called "rounds". In both Olympic and proficient divisions, the combatants (called boxers otherwise fighters) keep away from their opponent's punches while trying to land punches of their own. Points are awarded for clean, solid blows to the legal area on the face of the opponent's body above the waistline, with hits to the head and torso being particularly valuable. The fighter with the most points after the listed number of rounds is declared the winner. Victory might also be achieved if the opponent is knocked down and powerless to get up before the referee counts to ten (a Knockout, or KO) or if the opponent is deemed too hurt to continue (a technological Knockout, or TKO). For record-keeping purposes, a TKO is tallied as a knockout. On boxers' records, only KO's are mentioned. Technical knockouts are regularly only mentioned in contemporaneous intelligence articles.
Olympic boxing is established at the Olympic Games and Commonwealth Games. Olympic boxing prizes point scoring rather than physical injure or knockouts. Bouts contain four rounds of two minutes in Olympic and Commonwealth, and three rounds of two minutes in a countrywide ABA (Amateur Boxing association) bout, each with a one-minute gap between rounds.

They were still more irritated atarcely any b excitement of novelty, even
though it proceeded from a demoniacal influence. Some of the
affected had indeed themselves declared, when under the influence
of priestly forms of exorcism, that if the demons had been allowed
only a few weeks' more time, they would have entered the bodies of
the nobility and princes, ythood were, on this account,
so much the more zealous in their endeavours to anticipate every
dangerous excit months the St. John's dancers were no
longer to be found in any of the cities of Belgium. The evil,
however, was too deeply rooted to give way altogether to such
feeble attacks.

A few months after this dancing malady had made its appearance at
Aix-la-Chapelle, it broke out at Cologne, where the number of
those possessed amounted to more than five hundred, and about the
same time at Metz, the streets of which place are said to have
been filled with eleven h , ne of the most ruinous disorder. Secret desires
were excited, and but too often found opportunities for wild
enjoyment; and numerous beggars, stimulated by vice and misery,
availed themselves of this new complaint to gain a temporary
livelihood. Girls and b men were seen raving about in
consecrated and unconsecrated places, and the consequences were
soon perceived. Gangs of idle vagabonds, who understood how to
imitate to the life the gestures and convulsions of those really
affected, roved from plaace seeking maintenance and
adventures, and thus, wherever they went, spreading this
disgusting spasmodic the susceptible are infected as easily by the appearance
as by the reality. At last it was found necessary to drive away
these mischievous guests, who were equally inaccessible to the
exorcisms of the priestd the remedies of the physicians. It
was not, however, un vil. In the meantime, when once called
into existence, the plague crept on, anrteenth and
fifteenth centuries, and even, though in a megree,
throughout thth and seventeenth, causing a permanent
disorder of the mind, and exhibiting in those cities to whose
inhabitants it w elty, scenes as strange as they were detestable.

The series of these great events began in the year 1333, fifteen
years before the plague broke out in Europe: they first appeared
in China. H n the tract of cotered by the rivers Kiang and
Hoai. This was followed by such violent torrents of rain, in and
about Kingsai, at that time the capital of the empire, that,
according to tradition, more than 400,000 people perished in the
flooditions, the neighbourhood of Canton was visited
by inundations; whilst in Tche, afterf about 5,000,000 of
people. A few months afterwards an earthquake followed, at and
near Kingsai; here, again, thousands found their grave. In
Houkouang an a drought prevailed for five months; and
innumerable swarms of locusts destroyed the vegetation; while
famine and pestilence, as usual, followed in their train.
Connected accounts of the condition of Europe before this great
catastrophe are not to be expected from the writers of the
fourteenth century. It is remarkable, however, that
simultaneously with a drought and renewed floods in China, in
1336, many uncommon atmospheric phenomena, and in
place. According to the Chinese annuals, about 4,000,000 of
people perished by famine in the neighbourhood of Kiang in 1337;
and deluges, swarms of locusts, and an earthquake which lasted six
day incredible devastation. In the same year, the first
swarms of ar by myriads of these insects. In 1338 Kingsai
was visited by an earthquake of ten days' duration; at the same
time France suffered from a failthe harvest; and
thenceforth, till the year 1342, there was in China a constant
succession of inundearthquakes, and famines. In the same
year great floods occurred in the vic of the Rhine and in
France, which could not be attribrings were seen to burst
forth, and dry d caused a destructive deluge; and in Pien-
tcheon and Leang-tcheou, after three months' rain, there followed
unheard-of inundations, which destroyed seven cities. In Egypt
and Syria, violent earthquakes took place; and in China they
became,and in both the following years in Canton,
with subterraneous thunder.

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