A Mersenne prime is a Mersenne number, i.e., a number of the form
that is prime. In order for to be prime,
must itself be prime. This
is true since for composite
with factors
and
,
.
Therefore,
can be written as
,
which is a binomial number that always has a factor
.
The first few Mersenne primes are 3, 7, 31, 127, 8191, 131071, 524287, 2147483647, ... (OEIS A000668) corresponding to indices
, 3, 5, 7, 13, 17, 19, 31, 61, 89,
... (OEIS A000043).
Cataldi used his 1603 proper factor table to prove that
and
are prime (History of Mathematics Project n.d.).
Mersenne (1644) asserted that was prime for
, 3, 5, 7, 13, 17, 19, 31, 67, 127, and 257, but the list
contained five errors:
and
are composite, while the primes
,
, and
were omitted (Caldwell n.d.). Lucas (1876) proved that
was composite
using a Lucas sequence test, without finding a
factor. Cole (1903) famously presented the factorization
to the American Mathematical Society by silently performing the two sides of the calculation on a blackboard. He then sat down to applause (Cole 1903; Tattersall 1999, pp. 184-185). Lehmer's later refinement of Lucas's method is the modern Lucas-Lehmer test.
Japanese publisher Nanairosha has issued books whose hundreds of pages print the decimal digits of record Mersenne
primes, including
and
(National Diet Library 2018, 2021). Such books provide a striking physical visualization
of size, although base-10 expansion is a particularly uninformative representation
of these numbers. In binary, every Mersenne
number
is simply the repunit consisting of
ones.
Mersenne primes were first studied because of the remarkable property that every Mersenne prime corresponds to exactly one perfect number. L. Welsh maintains an extensive bibliography and history of Mersenne numbers.
It has been conjectured that there exist an infinite number of Mersenne primes. Fitting a line through the origin to the asymptotic number of Mersenne primes with
for the first 51 (known) Mersenne primes gives a best-fit
line with
,
illustrated above. If the line is not restricted to pass through the origin, the
best fit is
.
It has been conjectured (without any particularly strong evidence) that the constant
is given by
,
where
is the Euler-Mascheroni constant (Havil
2003, p. 116, Caldwell), a result related to Wagstaff's
conjecture.
However, finding Mersenne primes is computationally very challenging. For example, the 1963 discovery that
is prime was heralded by a special postal meter design, illustrated above, issued
in Urbana, Illinois.
In 1952, Raphael Robinson used the Standards Western Automatic Computer (SWAC) to discover the five Mersenne primes with exponents 521, 607, 1279, 2203, and 2281. The largest had 687 decimal digits, and the computation marked an early use of an electronic computer to extend the record for the largest known prime number (Robinson 1954).
G. Woltman has organized a distributed search program via the Internet known as GIMPS (Great Internet Mersenne Prime Search) in which hundreds of volunteers use
their personal computers to perform pieces of the search. The efforts of GIMPS volunteers
make this distributed computing project the discoverer of all of the Mersenne primes
discovered since late 1996. As of Sep. 7, 2026, GIMPS participants had tested
and verified all exponents below and tested all exponents below
at least once (GIMPS 2026).
The table below gives the index of known Mersenne primes (OEIS A000043)
, together with the number of digits,
discovery years, and discoverer. A similar table has been compiled by C. Caldwell.
As of Sep. 4, 2026, all smaller candidate exponents had been eliminated, establishing
as the 51st Mersenne prime.
The rank of the larger known Mersenne prime
remains provisional.
| # | digits | year | discoverer (reference) | value | |
| 1 | 2 | 1 | antiquity | 3 | |
| 2 | 3 | 1 | antiquity | 7 | |
| 3 | 5 | 2 | antiquity | 31 | |
| 4 | 7 | 3 | antiquity | 127 | |
| 5 | 13 | 4 | 1461 | Reguis (1536), Cataldi (1603) | 8191 |
| 6 | 17 | 6 | 1588 | Cataldi (1603) | 131071 |
| 7 | 19 | 6 | 1588 | Cataldi (1603) | 524287 |
| 8 | 31 | 10 | 1750 | Euler (1772) | 2147483647 |
| 9 | 61 | 19 | 1883 | Pervouchine (1883), Seelhoff (1886) | 2305843009213693951 |
| 10 | 89 | 27 | 1911 | Powers (1911) | 618970019642690137449562111 |
| 11 | 107 | 33 | 1913 | Powers (1914) | 162259276829213363391578010288127 |
| 12 | 127 | 39 | 1876 | Lucas (1876) | 170141183460469231731687303715884105727 |
| 13 | 521 | 157 | Jan. 30, 1952 | Robinson (1954) | 68647976601306097149...12574028291115057151 |
| 14 | 607 | 183 | Jan. 30, 1952 | Robinson (1954) | 53113799281676709868...70835393219031728127 |
| 15 | 1279 | 386 | Jun. 25, 1952 | Robinson (1954) | 10407932194664399081...20710555703168729087 |
| 16 | 2203 | 664 | Oct. 7, 1952 | Robinson (1954) | 14759799152141802350...50419497686697771007 |
| 17 | 2281 | 687 | Oct. 9, 1952 | Robinson (1954) | 44608755718375842957...64133172418132836351 |
| 18 | 3217 | 969 | Sep. 8, 1957 | Riesel | 25911708601320262777...46160677362909315071 |
| 19 | 4253 | 1281 | Nov. 3, 1961 | Hurwitz | 19079700752443907380...76034687815350484991 |
| 20 | 4423 | 1332 | Nov. 3, 1961 | Hurwitz | 28554254222827961390...10231057902608580607 |
| 21 | 9689 | 2917 | May 11, 1963 | Gillies (1964) | 47822027880546120295...18992696826225754111 |
| 22 | 9941 | 2993 | May 16, 1963 | Gillies (1964) | 34608828249085121524...19426224883789463551 |
| 23 | 11213 | 3376 | Jun. 2, 1963 | Gillies (1964) | 28141120136973731333...67391476087696392191 |
| 24 | 19937 | 6002 | Mar. 4, 1971 | Tuckerman (1971) | 43154247973881626480...36741539030968041471 |
| 25 | 21701 | 6533 | Oct. 30, 1978 | Noll and Nickel (1980) | 44867916611904333479...57410828353511882751 |
| 26 | 23209 | 6987 | Feb. 9, 1979 | Noll (Noll and Nickel 1980) | 40287411577898877818...36743355523779264511 |
| 27 | 44497 | 13395 | Apr. 8, 1979 | Nelson and Slowinski | 85450982430363380319...44867686961011228671 |
| 28 | 86243 | 25962 | Sep. 25, 1982 | Slowinski | 53692799550275632152...99857021709433438207 |
| 29 | 110503 | 33265 | Jan. 28, 1988 | Colquitt and Welsh (1991) | 52192831334175505976...69951621083465515007 |
| 30 | 132049 | 39751 | Sep. 20, 1983 | Slowinski | 51274027626932072381...52138578455730061311 |
| 31 | 216091 | 65050 | Sep. 6, 1985 | Slowinski | 74609310306466134368...91336204103815528447 |
| 32 | 756839 | 227832 | Feb. 19, 1992 | Slowinski and Gage | 17413590682008709732...02603793328544677887 |
| 33 | 859433 | 258716 | Jan. 10, 1994 | Slowinski and Gage | 12949812560420764966...02414267243500142591 |
| 34 | 1257787 | 378632 | Sep. 3, 1996 | Slowinski and Gage | 41224577362142867472...31257188976089366527 |
| 35 | 1398269 | 420921 | Nov. 12, 1996 | Joel Armengaud/GIMPS | 81471756441257307514...85532025868451315711 |
| 36 | 2976221 | 895832 | Aug. 24, 1997 | Gordon Spence/GIMPS | 62334007624857864988...76506256743729201151 |
| 37 | 3021377 | 909526 | Jan. 27, 1998 | Roland Clarkson/GIMPS | 12741168303009336743...25422631973024694271 |
| 38 | 6972593 | 2098960 | Jun. 1, 1999 | Nayan Hajratwala/GIMPS | 43707574412708137883...35366526142924193791 |
| 39 | 13466917 | 4053946 | Nov. 14, 2001 | Michael Cameron/GIMPS | 92494773800670132224...30073855470256259071 |
| 40 | 20996011 | 6320430 | Nov. 17, 2003 | Michael Shafer/GIMPS | 12597689545033010502...94714065762855682047 |
| 41 | 24036583 | 7235733 | May 15, 2004 | Josh Findley/GIMPS | 29941042940415717208...67436921882733969407 |
| 42 | 25964951 | 7816230 | Feb. 18, 2005 | Martin Nowak/GIMPS | 12216463006127794810...98933257280577077247 |
| 43 | 30402457 | 9152052 | Dec. 15, 2005 | Curtis Cooper and Steven Boone/GIMPS | 31541647561884608093...11134297411652943871 |
| 44 | 32582657 | 9808358 | Sep. 4, 2006 | Curtis Cooper and Steven Boone/GIMPS | 12457502601536945540...11752880154053967871 |
| 45 | 37156667 | 11185272 | Sep. 6, 2008 | Hans-Michael Elvenich/GIMPS | 20225440689097733553...21340265022308220927 |
| 46 | 42643801 | 12837064 | Jun. 12, 2009 | Odd Magnar Strindmo/GIMPS | 16987351645274162247...84101954765562314751 |
| 47 | 43112609 | 12978189 | Aug. 23, 2008 | Edson Smith/GIMPS | 31647026933025592314...80022181166697152511 |
| 48 | 57885161 | 17425170 | Jan. 25, 2013 | Curtis Cooper/GIMPS | 58188726623224644217...46141988071724285951 |
| 49 | 74207281 | 22338618 | Jan. 7, 2016 | Curtis Cooper/GIMPS | 30037641808460618205...87010073391086436351 |
| 50 | 77232917 | 23249425 | Dec. 26, 2017 | Jonathan Pace/GIMPS | 46733318335923109998...82730618069762179071 |
| 51 | 82589933 | 24862048 | Dec. 7, 2018 | Patrick Laroche/GIMPS | 14889444574204132554...37951210325217902591 |
| 52? | 136279841 | 41024320 | Oct. 12, 2024 | Luke Durant/GIMPS | 88169432750383326555...55076706219486871551 |
Trial division is often used to establish the compositeness of a potential Mersenne prime. This
test immediately shows
to be composite for
, 23, 83, 131, 179, 191, 239, and 251 (with small factors
23, 47, 167, 263, 359, 383, 479, and 503, respectively). A much more powerful primality
test for
is the Lucas-Lehmer test.
If
is a prime, then
divides
iff
is prime. It is also true
that prime divisors of
must have the form
where
is a positive integer
and simultaneously of either the form
or
(Uspensky and Heaslet 1939).
A prime factor of a Mersenne number
is a Wieferich prime iff
. Therefore, Mersenne primes are not Wieferich
primes.
