Mersenne prime (original) (raw)
A Mersenne prime is a prime number that is one less than a power of two. For example, 3 = 4 − 1 = 22 − 1 is a Mersenne prime; so is 7 = 8 − 1 = 23 − 1. On the other hand, 15 = 16 − 1 = 24 − 1, for example, is not a prime. Fast algorithms for finding Mersenne primes are available, and this is why the largest known prime numbers today are Mersenne primes.
Mersenne primes have a close connection to perfect numbers, which are numbers that are equal to the sum of their proper divisors. Historically, the study of Mersenne primes was motivated by this connection; in the 4th century BC Euclid demonstrated that if M is a Mersenne prime then M(M+1)/2 is a perfect number. Two millennia later, in the 18th century, Euler proved that all even perfect numbers have this form. No odd perfect numbers are known, and it is suspected that none exist.
It is currently unknown whether there is an infinite number of Mersenne primes.
More generally, Mersenne numbers (not necessarily primes, but candidates for primes) are numbers that are one less than an odd power of two; the notation Mn = 2_n_ − 1 is used. The calculation
shows that Mn can be prime only if n itself is prime, which simplifies the search for Mersenne primes considerably. But the converse is not true; Mn may be composite even though n is prime. For example, 211 − 1 = 23 · 89.
The first four Mersenne primes _M_2, _M_3, _M_5, _M_7 were known in antiquity. The fifth, _M_13, was discovered anonymously before 1461; the next two (_M_17 and _M_19) were found by Cataldi in 1588. After more than a century _M_31 was verified to be prime by Euler in 1750. The next (in historical, not numerical order) was _M_127, found by Lucas in 1876, then _M_61 by Pervushin in 1883. Two more - _M_89 and _M_107 - were found early in the 20th century, by Powers in 1911 and 1914, respectively.
The numbers are named after 17th century French mathematician Marin Mersenne, who provided a list of Mersenne primes with exponents up to 257; unfortunately, his list was not correct, though, as he mistakenly included _M_67 and _M_257, and omitted _M_61, _M_89 and _M_109.
The best method presently known for testing the primality of Mersenne numbers is based on the computation of a recurring sequence, as developed originally by Lucas in 1878 and improved by Lehmer in the 1930s, now known as the Lucas-Lehmer test. Specifically, it can be shown that Mn = 2_n_ − 1 is prime if and only if Mn evenly divides Sn-2, where _S_0 = 4 and for k > 0, S k = S k − 12 − 2.
The search for Mersenne primes was revolutionized by the introduction of the electronic digital computer. The first successful identification of a Mersenne prime, _M_521, by this means was achieved at 10:00 P.M. on January 30, 1952 using the U.S. National Bureau of Standards Western Automatic Computer (SWAC) at the Institute for Numerical Analysis at the University of California, Los Angeles, under the direction of Lehmer, with a computer search program written and run by Prof. R.M. Robinson. It was the first Mersenne prime to be identified in thirty-eight years; the next one, _M_607, was found by the computer a little less than two hours later. Three more - _M_1279, _M_2203, _M_2281 - were found by the same program in the next several months.
As of December 2003, only 40 Mersenne primes were known; the largest known prime number (220,996,011 − 1) is a Mersenne prime. Like several previous Mersenne primes, it was discovered by a distributed computing project on the Internet, known as the Great Internet Mersenne Prime Search (GIMPS). The table below lists all known Mersenne primes (also confer Sloane's A000043):
# | p | Digits in M p | Date of discovery | Discoverer |
---|---|---|---|---|
1 | 2 | 1 | ancient | ancient |
2 | 3 | 1 | ancient | ancient |
3 | 5 | 2 | ancient | ancient |
4 | 7 | 3 | ancient | ancient |
5 | 13 | 4 | 1456 | anonymous |
6 | 17 | 6 | 1588 | Cataldi |
7 | 19 | 6 | 1588 | Cataldi |
8 | 31 | 10 | 1772 | Euler |
9 | 61 | 19 | 1883 | Pervushin |
10 | 89 | 27 | 1911 | Powers |
11 | 107 | 33 | 1914 | Powers |
12 | 127 | 39 | 1876 | Lucas |
13 | 521 | 157 | 1952 | Robinson |
14 | 607 | 183 | 1952 | Robinson |
15 | 1,279 | 386 | 1952 | Robinson |
16 | 2,203 | 664 | 1952 | Robinson |
17 | 2,281 | 687 | 1952 | Robinson |
18 | 3,217 | 969 | 1957 | Riesel |
19 | 4,253 | 1,281 | 1961 | Hurwitz |
20 | 4,423 | 1,332 | 1961 | Hurwitz |
21 | 9,689 | 2,917 | 1963 | Gillies |
22 | 9,941 | 2,993 | 1963 | Gillies |
23 | 11,213 | 3,376 | 1963 | Gillies |
24 | 19,937 | 6,002 | 1971 | Tuckerman |
25 | 21,701 | 6,533 | 1978 | Noll & Nickel |
26 | 23,209 | 6,987 | 1979 | Noll |
27 | 44,497 | 13,395 | 1979 | Nelson & Slowinski |
28 | 86,243 | 25,962 | 1982 | Slowinski |
29 | 110,503 | 33,265 | 1988 | Colquitt & Welsh |
30 | 132,049 | 39,751 | 1983 | Slowinski |
31 | 216,091 | 65,050 | 1985 | Slowinski |
32 | 756,839 | 227,832 | 1992 | Slowinski & Gage |
33 | 859,433 | 258,716 | 1994 | Slowinski & Gage |
34 | 1,257,787 | 378,632 | 1996 | Slowinski & Gage |
35 | 1,398,269 | 420,921 | November 13 1996 | GIMPS / Joel Armengaud |
36 | 2,976,221 | 895,932 | August 24 1997 | GIMPS / Gordon Spence |
37 | 3,021,377 | 909,526 | January 27 1998 | GIMPS / Roland Clarkson |
38 | 6,972,593 | 2,098,960 | June 1 1999 | GIMPS / Nayan Hajratwala |
39? | 13,466,917 | 4,053,946 | November 14 2001 | GIMPS / Michael Cameron (Canada) |
40? | 20,996,011 | 6,320,430 | November 17 2003 | GIMPS / Michael Shafer |
See also
External links
- Mersenne prime section of the Prime Pages: http://www.utm.edu/research/primes/mersenne.shtml
- Mersenne Prime Search home page: http://www.mersenne.org