Now we are looking on the crossword clue for: “Word that can follow “”South”” or “”ski”””.
it’s A 103 letters crossword puzzle definition.
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Possible Answers:
Pole.
Last seen on: Daily Celebrity Crossword – 6/23/19 People Sunday
Random information on the term ““Word that can follow “”South”” or “”ski””””:
E (named e /iː/, plural ees) is the fifth letter and the second vowel in the modern English alphabet and the ISO basic Latin alphabet. It is the most commonly used letter in many languages, including Czech, Danish, Dutch, English, French, German, Hungarian, Latin, Latvian, Norwegian, Spanish, and Swedish.
The Latin letter ‘E’ differs little from its source, the Greek letter epsilon, ‘Ε’. This in turn comes from the Semitic letter hê, which has been suggested to have started as a praying or calling human figure (hillul ‘jubilation’), and was probably based on a similar Egyptian hieroglyph that indicated a different pronunciation. In Semitic, the letter represented /h/ (and /e/ in foreign words); in Greek, hê became the letter epsilon, used to represent /e/. The various forms of the Old Italic script and the Latin alphabet followed this usage.
Although Middle English spelling used ⟨e⟩ to represent long and short /e/, the Great Vowel Shift changed long /eː/ (as in ‘me’ or ‘bee’) to /iː/ while short /ɛ/ (as in ‘met’ or ‘bed’) remained a mid vowel. In other cases, the letter is silent, generally at the end of words.
“Word that can follow “”South”” or “”ski””” on Wikipedia
Random information on the term “Pole”:
The north and south celestial poles are the two imaginary points in the sky where the Earth’s axis of rotation, indefinitely extended, intersects the celestial sphere. The north and south celestial poles appear permanently directly overhead to an observer at the Earth’s North Pole and South Pole, respectively. As the Earth spins on its axis, the two celestial poles remain fixed in the sky, and all other points appear to rotate around them, completing one circuit per day (strictly, per sidereal day).
The celestial poles are also the poles of the celestial equatorial coordinate system, meaning they have declinations of +90 degrees and −90 degrees (for the north and south celestial poles, respectively).
The celestial poles do not remain permanently fixed against the background of the stars. Because of a phenomenon known as the precession of the equinoxes, the poles trace out circles on the celestial sphere, with a period of about 25,700 years. The Earth’s axis is also subject to other complex motions which cause the celestial poles to shift slightly over cycles of varying lengths; see nutation, polar motion and axial tilt. Finally, over very long periods the positions of the stars themselves change, because of the stars’ proper motions.