495 (number)
| ||||
---|---|---|---|---|
Cardinal | four hundred ninety-five | |||
Ordinal |
495th (four hundred and ninety-fifth) | |||
Factorization | 32× 5 × 11 | |||
Roman numeral | CDXCV | |||
Binary | 1111011112 | |||
Ternary | 2001003 | |||
Quaternary | 132334 | |||
Quinary | 34405 | |||
Senary | 21436 | |||
Octal | 7578 | |||
Duodecimal | 35312 | |||
Hexadecimal | 1EF16 | |||
Vigesimal | 14F20 | |||
Base 36 | DR36 |
495 is the integer after 494 and before 496. It is a pentatope number[1] (and so a binomial coefficient ).
Kaprekar transformation
The Kaprekar transformation is defined as follows for three-digit numbers:
- Start with a three-digit number with at least two digits different.
- Arrange the digits in ascending and then in descending order to get two three-digit numbers, adding leading zeros if necessary.
- Subtract the smaller number from the bigger number.
- Go back to step 2.
Repeating this process will always reach 495 in a few steps. Once 495 is reached, the process stops because 954 – 459 = 495.
Example
For example, choose 589:
- 985 − 589 = 396
- 963 − 369 = 594
- 954 − 459 = 495
The only three-digit numbers for which this function does not work are repdigits such as 111, which give the answer 0 after a single iteration. All other three-digits numbers work if leading zeros are used to keep the number of digits at 3:
- 211 – 112 = 099
- 990 – 099 = 891 (rather than 99 - 99 = 0)
- 981 – 189 = 792
- 972 – 279 = 693
- 963 – 369 = 594
- 954 − 459 = 495
The number 6174 has the same property for the four-digit numbers.
See also
- Collatz conjecture — sequence of unarranged-digit numbers always ends with the number 1.
References
- ↑ "Sloane's A000332". The On-Line Encyclopedia of Integer Sequences. OEIS Foundation. Retrieved 2016-05-16.
- Eldridge, Klaus E.; Sagong, Seok (February 1988). "The Determination of Kaprekar Convergence and Loop Convergence of All Three-Digit Numbers". The American Mathematical Monthly. The American Mathematical Monthly, Vol. 95, No. 2. 95 (2): 105–112. doi:10.2307/2323062. JSTOR 2323062.
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