MAGIC SQUARE: Calculate A+B+C
[6047] MAGIC SQUARE: Calculate A+B+C - The aim is to place the some numbers from the list (3, 4, 8, 10, 20, 21, 25, 71, 72, 76) into the empty squares and squares marked with A, B an C. Sum of each row and column should be equal. All the numbers of the magic square must be different. Find values for A, B, and C. Solution is A+B+C. - #brainteasers #math #magicsquare - Correct Answers: 14 - The first user who solved this task is Nasrin 24 T
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MAGIC SQUARE: Calculate A+B+C

The aim is to place the some numbers from the list (3, 4, 8, 10, 20, 21, 25, 71, 72, 76) into the empty squares and squares marked with A, B an C. Sum of each row and column should be equal. All the numbers of the magic square must be different. Find values for A, B, and C. Solution is A+B+C.
Correct answers: 14
The first user who solved this task is Nasrin 24 T.
#brainteasers #math #magicsquare
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Tailor-made suit

A young banker decided to get his first tailor-made suit. So he went tothe finest tailor in town and got measured for a suit. A week later hewent in for his first fitting. He put on the suit and he looked fabulous,he felt that in this suit he can do business.

As he was preening himself in front of the mirror he reached down to puthis hands in the pockets and to his surprise he noticed that there were nopockets. He mentioned this to the tailor who asked him, "Didn't you tellme you were a banker?"

The young man answered, "Yes, I did."

To this the tailor said, "Whoever heard of a banker with his hands in hisown pockets?"

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Hendrik Christoffel Van de Hulst

Born 19 Nov 1918; died 31 Jul 2000 at age 81.Dutch astronomer who predicted theoretically (1944) that in interstellar space the amount of neutral atomic hydrogen, which in its hyperfine transition radiates and absorbs at a wavelength of 21 cm, might be expected to occur at such high column densities as to provide a spectral line sufficiently strong as to be measurable. Shortly after the end of the war several groups set about to test this prediction. The 21-cm line of atomic hydrogen was detected in 1951, first at Harvard University followed within a few weeks by others. The discovery demonstrated that astronomical research, which at that time was limited to conventional light, could be complemented with observations at radio wavelengths, revealing a range of new physical processes.
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