Algol A is about 3.7 times as massive as the Sun, while Algol B has a mass of only 0.8 solar masses. According to stellar evolution theory, a more massive star evolves more rapidly; yet in the Algol system the more massive Algol A is still a main-sequence star while Algol B has evolved to become a subgiant. This is the Algol paradox, which is explained by slow and continuous mass transfer from Algol B to Algol A (see Algol variables). This mass transfer, along with apsidal motion, accounts for slight changes in the time of Algol's eclipses. The streams of gas passing from Algol B to Algol A make Algol an erratic radio and X-ray source. mv : 2.1 (A), 3.5 (B); Mv : –0.2 (A), 1.2 (B); spectral type: B8 V (A), K0 IV (B); distance: 29 pc.
fahrenheit begin real fahr; print ("Enter Fahrenheit "); read (fahr); print ("Celsius is ",(fahr-32.0)*5.0/9.0); end finish
an abbreviated name denoting a series of programming languages formed from the initial letters of the English words “algorithmic” and “language.” ALGOL was devised by an international group of scientists in 1958–60. The final form of the language, as adopted by an international conference of January 1960 in Paris, was given the name ALGOL-60 to distinguish it from the initial version, called ALGOL-58.
The basic symbols of ALGOL are decimal digits, upper and lowercase letters of the alphabet, punctuation marks, symbols of mathematical and logical operations, and various other special signs, as well as certain English words (in particular, “begin” and “end”). From the basic ALGOL symbols, following definite rules, constructions are formed —numbers and expressions (arithmetic, logical, and others), descriptions, notes, and operators; these operators, in turn, in combination with the basic symbols, combine to form more complicated operators, and so on. An algorithm assigned in ALGOL is a so-called ALGOL program. With the help of a second special program it is transformed into a program in the language of the particular digital computer.