Calculate the number 6698
[3162] Calculate the number 6698 - NUMBERMANIA: Calculate the number 6698 using numbers [6, 4, 9, 3, 15, 656] and basic arithmetic operations (+, -, *, /). Each of the numbers can be used only once. - #brainteasers #math #numbermania - Correct Answers: 34 - The first user who solved this task is Djordje Timotijevic
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Calculate the number 6698

NUMBERMANIA: Calculate the number 6698 using numbers [6, 4, 9, 3, 15, 656] and basic arithmetic operations (+, -, *, /). Each of the numbers can be used only once.
Correct answers: 34
The first user who solved this task is Djordje Timotijevic.
#brainteasers #math #numbermania
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More Halloween 2018 jokes

What plants like Halloween the most?
Bam-BOO!

What do birds say on Halloween?
Twick or tweet

What do you get when you cross a werewolf and a vampire?
A fur coat that fangs around your neck.

What would you find on a haunted beach?
A sand-witch!

Why didn’t the skeleton like the Halloween candy?
He didn’t have the stomach for it!

What’s worse than being a five-ton witch on Halloween?
Being her broom!

Why do ghosts like to ride in elevators?
It raises their spirits.

What do you get when you divide the circumference of a jack-o-lantern by its diameter?
Pumpkin Pi.

What would you get if you crossed a vampire and a teacher?
Lots of blood tests!

Why are vampires so easy to fool?
Because they’re suckers.

What did the ghost say when the skeleton lied to him?
I can see right through you.

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Comet

In 1864, Giovanni Batista Donati (1827-73) made the first spectroscopic observations of a comet tail (from the small comet, Tempel, 1864 II). At a distance from the Sun the spectrum of a comet is identical to that of the Sun, and its visibility is due only to reflected sunlight. Donati showed that comet tail formed close to the Sun contains luminous gas. In the spectrum of light from the comet tail, Donati saw three absorption lines bands superimposed on a continuous spectrum, which he named alpha, beta and gamma, and are now known as the Swan bands. These bands were also seen in a comet tail viewed by Pietro Secchi in 1866. Sir William Huggins (1868) identified that these were due to the presence of carbon (molecular carbon, C2).[Image: Comet tail of Comet West 1976 VI, computer generated false colour image.]
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