CINEMANIA: Guess the movie title
[4745] CINEMANIA: Guess the movie title - See negative of movie scene and guess the title. Length of words in solution: 4 - #brainteasers #movie #film #cinemania - Correct Answers: 16 - The first user who solved this task is Djordje Timotijevic
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CINEMANIA: Guess the movie title

See negative of movie scene and guess the title. Length of words in solution: 4
Correct answers: 16
The first user who solved this task is Djordje Timotijevic.
#brainteasers #movie #film #cinemania
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Private Audience With the Holy Mother

After a long life of unselfish service, Father John O'Malley died and went to heaven. St. Peter met him at the gate and said: "John, you did such a wonderful job for us on earth, we'd like to do something special for you. You name it; it's yours."
John thought for a moment and said: "I'd like a private audience with the Holy Mother." St. Peter told him it would be arranged.On the appointed day, St. Peter escorted John to the Holy Mother's sanctuary. John went before Her, knelt, and said: "Holy Mother, I've always looked to You for guidance, and You have granted me peace and serenity through some difficult times. But I have one question that has nagged me during my whole time on earth. In all the paintings that were done of you, and in all the sculptures that were carved of you, you always looked so sad. Why is that?"
Mary thought for a moment, pursing her lips. She said: "I always wanted a girl."

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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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