Calculate the number 7456
[8147] Calculate the number 7456 - NUMBERMANIA: Calculate the number 7456 using numbers [6, 6, 8, 3, 52, 609] and basic arithmetic operations (+, -, *, /). Each of the numbers can be used only once. - #brainteasers #math #numbermania - Correct Answers: 0
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Calculate the number 7456

NUMBERMANIA: Calculate the number 7456 using numbers [6, 6, 8, 3, 52, 609] and basic arithmetic operations (+, -, *, /). Each of the numbers can be used only once.
Correct answers: 0
#brainteasers #math #numbermania
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No room at the inn

By the time the sailor pulled into a little town every hotel room was taken. "You've got to have a room somewhere," he pleaded. "Or just a bed, I don't care where."

"Well, I do have a double room with one occupant - an Air Force guy," admitted the manager, "and he might be glad to split the cost. But to tell you the truth, he snores so loudly that people in adjoining rooms have complained in the past.

I'm not sure it'd be worth it to you."

"No problem," the tired Navy man assured him. "I'll take it." The next morning, the sailor came down to breakfast bright-eyed and bushy tailed. "How'd you sleep?" asked the manager. "Never better." The manager was impressed. "No problem with the other guy snoring?" "Nope. I shut him up in no time," said the Navy guy.

"How'd you manage that?" asked the manager.

"He was already in bed, snoring away, when I came in the room," the sailor explained. "I went over, gave him a kiss on the cheek, and said, 'Goodnight beautiful,'

...and he sat up all night watching me."

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Subrahmanyan Chandrasekhar

Died 21 Aug 1995 at age 84 (born 19 Oct 1910). Indian-American astronomer and astrophysicist who shared (with William A.Fowler) the 1983 Nobel Prize for Physics for formulating the currently accepted theory on the later evolutionary stages of massive stars (which has led to the discovery of black holes and neutron stars). He was one of the first scientists to combine the disciplines of physics and astronomy. Early in his career he demonstrated that there is an upper limit, now called the Chandrasekhar limit, to the mass of a white dwarf star. (A white dwarf is the last stage in the evolution of a star such as the Sun, which ends with collapse when the nuclear energy source in its centre has become exhausted.) Further, it shows that stars much more massive than the Sun must either explode or form black holes.
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