Rules
Guess the NERDLE in 6 tries. After each try, the color of the tiles will change to show how close your guess is to the solution.
If the tile becomes GREEN, your number or operation is located at correct place. If the tile becomes RED, your number or opeartion exists within the expression, but at different place.
- Each try is a calculation (math expression).
- You can use 0 1 2 3 4 5 6 7 8 9 + - * / or =.
- It must contain one “=”.
- It must only have a number to the right of the “=”, not another calculation.
- Standard order of operations applies, so calculate * and / before + and - eg. 3+2*5=13 not 25!
Example of the correct math expression:
Joke Of The Day
Hubby: You always carry my pho...
Hubby: You always carry my photo in your handbag to the office. Why?
Wife: When there is a problem, no matter how impossible, I look at your picture and the problem disappears.
Hubby: You see, how miraculous and powerful I am for you?
Wife: Yes, I see your picture and say to myself, "What other problem can there be greater than this one?"
Wife: When there is a problem, no matter how impossible, I look at your picture and the problem disappears.
Hubby: You see, how miraculous and powerful I am for you?
Wife: Yes, I see your picture and say to myself, "What other problem can there be greater than this one?"
Source: JokesOfTHeDay.net - Brain Teasers Partner
On This Day
John Henry PoyntingBorn 9 Sep 1852; died 30 Mar 1914 at age 61.British physicist who introduced a theorem (1884-85) that assigns a value to the rate of flow of electromagnetic energy known as the Poynting vector, introduced in his paper On the Transfer of Energy in the Electromagnetic Field (1884). In this he showed that the flow of energy at a point can be expressed by a simple formula in terms of the electric and magnetic forces at that point. He determined the mean density of the Earth (1891) and made a determination of the gravitational constant (1893) using accurate torsion balances. He was also the first to suggest, in 1903, the existence of the effect of radiation from the Sun that causes smaller particles in orbit about the Sun to spiral close and eventually plunge in. |
This site uses cookies to store information on your computer. Some are essential to help the site properly. Others give us insight into how the site is used and help us to optimize the user experience. See our privacy policy.
