Notable Properties of Specific Numbers  


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247

247 is an Eulerian number. The Eulerian numbers, given by Sloane's A0295, begin: 0, 1, 4, 11, 26, 57, 120, 247, 502, 1013, 2036, ... and are simply the values of 2n-n-1. These numbers usually manifest themselves as a permutation count. In this figure, each of the permutations has exactly one place where a larger number follows a smaller number (called an "ascent"):

A[2] = 1   12

A[3] = 4   132 213 231 312

A[4] = 11   1432 2143 2431 3142 3214 3241 3421 4132 4213 4231 4312

The Eulerian numbers show up as the first non-trivial diagonal of a number triangle (called Euler's triangle) that is like Pascal's triangle, but with rows that add up to successive factorials:

1 sum: 1 1 1 sum: 2 1 4 1 sum: 6 1 11 11 1 sum: 24 1 26 66 26 1 sum: 120 1 57 302 302 57 1 sum: 720 1 120 1191 2416 1191 120 1 sum: 5040 1 247 4293 15619 15619 4293 247 1 sum: 40320

To compute numbers in this triangle, you add the two numbers above it, each multiplied by the index number of the diagonal shared by that number. For example, consider the first 26 in the 4th row. The numbers 1 and 11 are above it. The 26 and the 11 share the 2nd diagonal, counting from the left, so we take 11×2. The 26 and the 1 are in the 4th diagonal, counting from the right, so we take 1×4. This gives 11×2 + 1×4, which is 26. For another example, 57×5 + 302×3 = 1191: the multipliers 5 and 3 are used because the number to be computed is in the 5th and 3rd diagonals.

The first few diagonals of the Euler triangle are A0295, A0460, and A0498, and the largest number in each row is given by A6551. All of these count permutations, but with different requirements for how many "ascents" there are.

2:47 is 13×19, but you're six minutes late.

251

251 is the first of a set of 4 consecutive primes that are spaced an equal distance apart: 251, 257, 263, and 269 are all prime, there are no primes in between, and the spacing between them is 6. 251 is the lowest number with this property; the next is 1741. See also 47, 9843019, 121174811 and 19252884016114523644357039386451.

252 = 10×9×8×7×6 / (5×4×3×2×1)

If you flip a coin 10 times in a row, there are exactly 252 ways in which it can turn out that you get exactly 5 heads and 5 tails (some examples are HTHTTTTHHH, THTHTHTHTH, HHHHHTTTTT, TTHHHHTHTT). Note the rather elegant way of expressing this using the numbers 1 through 10. This type of expression can be used to calculate any of the numbers down the center of Pascal's triangle. See also 2520.

256

This is 28, and is the number of possible values that can be stored in a byte, the most common unit of measurement for computer memory quantities. The number of values results from the fact that there are eight bits in a byte, and each bit can have two values (0 or 1). (Yes, during one period of history (16th century and earlier) there were also eight "bits" in a Spanish dollar, a fact that is related to the phrase "pieces of eight", and "two bits" (as in "shave and a haircut — two bits", slang for "25 cents"). The Spanish dollar was a gold coin with a value of eight reale, and was sometimes actually cut into eight wedge-shaped pieces to make change.)

Eight bits became the standard computer memory quantity because it is also a power of 2 (other smaller "bytes" were used in the early days when memory was expensive, but having the number of bits be a power of two makes many operations more efficient.) The next smaller power-of-2 size would be 4 bits per "byte", but that only allows for 16 = 24 possible byte values. The need to store and manipulate text, including a full alphabet (26 characters in the country where most of the computers were being developed) plus digits and many punctuation symbols meant that a byte that takes at least 100 or so values was necessary.

If computers had been developed in one of the many countries that have over 256 writing symbols (those that use the Korean, Ethiopic, Japanese, Chinese, and Vietnamese writing systems, among others) they might well have settled on a 16-bit byte. In fact, the emerging world standard for text (Unicode) uses 16-bit character codes, and allows distinct values for every symbol in every popular writing system.

257 = 223+1

(a Fermat number)

257 is a Fermat number, a number of the form 22N+1. Fermat hypothesized that all of these were prime, but they are not. A discussion of them and their factors is here. See also 641.

(Personal: the course number of my only Men's Weekend production)

260 = 13×20

The number of days in the tzol k'in, the almanac cycle Mayans used for divination (a system that originated at least 2600 years ago and is still used by native Americans in Yucatan, Guatemala, Belize, and Honduras). The days in the tzol k'in have successive names from a set of 20 (similar to the 20 days in the Mayan civil week) and numbers from a set of 13. There are thus 13×20 combinations of a name and a number and it takes this many days for the cycle to repeat, so the days were effectively named by a base {13,20} residue number system. It is not known why 260 was "chosen" although there are many theories. It is well-known the Mayans recognized a period of 52×365 days (slightly less than 52 tropical years), which is exactly equal to 18980=73×260 days, with 73 being exactly a fifth of 365 — but this cycle does not line up with other important astronomical periods (including the eclipse seasons, the lunar month and the synodic period of Venus, each of which was well-known and considered very important). See also 5126 and 1872000.

284

See 220.

288 = 4!×3!×2!×1! = 44+33+22+11

(4 superfactorial by the Sloane-Plouffe definition)

This is the value of "4 superfactorial" by the lower (Sloane and Plouffe 1995) definition of "superfactorial": 4!×3!×2!×1! = 24×6×2 = 288. By a rather nifty coincidence, it is also equal to 44+33+22+11 = 256+27+8+1.

Barnes' G-function

Barnes' G-function is to superfactorials as the Gamma function is to normal factorials. Barnes' G-function can be (very slowly) calculated by the formula:

G(z) = 2πz/2 e-[z(z+1)+γ z2]/2 PRODUCT(n=1..inf)[(1+z/n)n e-z+z2/(2n)]

where γ is the Euler-Mascheroni constant. For sufficiently large values of z you can use the approximation:

G(n) ≈ (e1/12/A) nn2/2-1/12(2π)n/2e-3n2/4

where A is the Glaisher-Kinkelin constant. See the MathWorld page 86 for more.

See also 1010102.0691973765×1036305. There is also a hyperfactorial.

298.257223563

The reciprocal of the oblateness of the Earth according to the WGS 84 model. The diameter of the Earth measured through the equator exceeds the polar diameter by about 1/298.26 of its size. In other words, if P is the polar diameter and E is the equatorial diameter, then (E-P)/E ≈ 1/298.26. WGS 84 is an approximation of the Geoid, which is a "gravitational equipotential surface".

See also 6378137.

304

I recently moved, and my house number changed from 27 to 304. I wanted to find relationships between these two numbers, and quickly found two rather straightforward ones:

304 = 3 × 10 × 10 + 4   and   27 = 3 + 10 + 10 + 4 (change × to +)

304 = 24 × 19   and   27 = 2 × 4 + 19 (change ^ to × and × to +)

This sort of thing is very common.

323

323 is a Motzkin number; see 51.

323 = 17×19, a product of two primes that, together with 1001 and 2001, create the rather nice digit pattern of the primorial 6469693230.

325

325 = 182+12 = 172+62 = 152+102, and is the smallest number that can be expressed as the sum of two distinct positive squares in at least 3 different ways. The sequence of such numbers is: 5, 65, 325, 1105, 5525, 27625, 71825, ... (Sloane's A52199; see also A93195). An interesting thing about these numbers is that all of their factors are prime numbers of the form 4n+1 (5, 13, 17, 29, 37, ... the "Pythagorean primes" A2144), and their factorizations are similar to those of the highly composite numbers. See also 1729 and 635318657.

327

(a perfect totient number)

327 is a perfect totient number. This is like a perfect number, but adding together the iterates of the totient function instead of adding together the number's factors. The Euler totient function, Sloane's A0010, counts how many numbers smaller than N are relatively prime to N. For example, if N is 14, the numbers 1, 3, 5, 9, 11 and 13 are relatively prime (notice that 1 counts), so the totient function of 14 is 6. For a prime P we're counting all numbers smaller than P, which is P-1, so the totient function always gives a smaller number except (by definition) when N=1. So, we can take a number like 327, and compute the Totient function (which gives 216), then compute the totient function of that number, and so on (giving 72, 24, 8, 4, 2 and 1), then add all these numbers together and we get 216 + 72 + 24 + 8 + 4 + 2 + 1 = 327. There is more about these numbers on a separate page here; see also 243.

327 also "combines" two of my favorite numbers, 3 and 27. When watching a baseball game I immediately notice when a batter's average or some similar statistic is .327, but it seems to happen more often then random chance would allow (.327 results from a record of 17 for 52, or a multiple like 34 for 104). This is the cult number effect in action.

336

(3-D oblong number)

A "3-dimensional oblong number", the volume of a rectangular solid of dimensions 6×7×8. If you add the middle number (7) you get 73=343. Numbers of this type are always a multiple of 6, because in any three consecutive integers there is always exactly one multiple of 3 and at least one even number. The sequence starts: 6, 24, 60, 120, 210, 336, 504, 720, 990, 1320, 1716, ... (Sloane's A7531).

A "generalized oblong number" is the product of 2 or more consecutive positive integers. These include the regular oblong numbers, 3-way products such as 336, and numbers like 120 formed by the product of 4 or more integers. The sequence starts: 2, 6, 12, 20, 24, 30, 42, 56, 60, 72, 90, 110, 120, 132, 156, 182, 210, 240, 272, 306, 336, 342, 360, 380, 420, 462, 504, 506, 552, 600, ... (Sloane's A45619). Each is the value of nPr for some values of n and r, n>r and r>1.

341

For all prime numbers p (except 2), 2p modulo p is 2:

3 is prime, 23 = 8 = 3×2+2
5 is prime, 25 = 32 = 5×6+2
7 is prime, 27 = 128 = 7×18+2
11 is prime, 211 = 2048 = 11×186+2
13 is prime, 213 = 8192 = 13×630+2
etc.

This is also true for some (but only a very few) composite numbers. The first composite number for which it is true is 341 = 11 × 31.

Checking a number p by this method is called a primality test because it allows you to quickly find out if a number is composite. The same method works with other bases in place of 2, as long as the base and p have no common factors. In the case of base 2, this means checking if p is odd or even. 341 "fools the test" for base 2 because it gives the same result a prime number would: 2341 is 2 modulo 341. However, it doesn't fool the test for base 3: 3341 is 168 modulo 341. See 561 for more.

341 is also 143 backwards.

343

343 equals 73 = 35 + 102

343 = (3+4)3, a "Friedman number"

and (tragically) it is the number of New York City firefighters killed at the World Trade Center on 2001 Sep 11th.

347

347 = 73+4, and is therefore able to be expressed in two different ways using the same 3 digits (3, 4 and 7). This is called a Friedman number.

360

360 can be evenly divided in 24 different ways — more than any other number of this size (see this entry for more about this).

360 is the number of degrees in a full circle. This size for angular division was chosen by the Babylonians because it is 602/10 and because it is close to the distance the sun moves through the zodiac each day (in other words, it is close to the length of the tropical year. In N days, the sun moves just about N degrees across the zodiac.

Conveniently for us Earthlings, the number of days per year happens to be pretty darn close to 360, a number with lots of factors. This means that, for lots of fairly common divisions (like 1/3 of a year, 1/4 of a year, etc.) it's pretty easy to remember how many days is involved because it's so close to what you'd get if the number were exactly 360. Thus: a quarter-year is just about 90 days; etc. For more accuracy you can easily add the fraction of the remaining 5 (e.g. adding 1.25 days to get 91.25 as a better approximation for the quarter-year).

See also 3600 and 3603600.

364.4

(Smoots from Nowhere to Hell)

Length of the Harvard Bridge in Boston (which actually bridges Boston to M.I.T. and is nowhere near Harvard University), measured in "smoots". In October 1958, as a fraternity prank, then-freshman Oliver Smoot (MIT class of 1962) was used as a unit of measurement to measure the length of the bridge (which MIT students use to walk to and from Boston.) Appropriately, Smoot went on in life to eventually serve as President of the International Organization for Standardization (ISO), and as chairman of the American National Standards Institute (ANSI).

His height at the time, 5 feet 7 inches, is a fairly well known "nonstandard unit" of length measurement. It is available in Google's built-in calculator (type "27 feet in smoots" in any Google search box) and as an optional unit in Google Earth (in the Ruler tool). The markings themselves are so well-accepted by the public that when the bridge was replaced in the 1980s, the Cambridge Police department requested that the markings be maintained, since they had become useful for identifying the location of accidents on the bridge. The construction crew went one better, by actually scoring the concrete surface of the sidewalk on the bridge at 1-smoot intervals instead of something more conventional, like 4 or 6 feet (see here).

365

Often used in quick and sloppy calculations as the number of days in a year. 365 is 52 weeks plus one day.

The ancient Mayan and Egyptian cultures each (independently) came up with calendars that divided most of the year into equal-sized months (18×20 or 12×30 days respectively) and then added a 5- or 6-day intercalary period.

The Egyptian calendar is still in use within the Coptic Orthodox church in Egypt; the 5-6 day period is called Pi Kogi Enavot and falls in the second week of September.

The Mayan 365-day count (called Haab') is still kept by indigenous peoples in Guatemala and nearby parts of Mexico. It was known to the early Mesoamericans that this was not an accurate approximation; see 550420.


The Tropical Year

The tropical year is the amount of time for the Earth to complete one orbit around the Sun, measured from equinox to equinox or from solstice to solstice. It differs from the sidereal year because of the Earth's axial precession and the effects of other planets.

This is the most important definition of "year" for most people because it is the ratio between the frequency of day and night (the average solar day) and the frequency of the seasons. It is the value that solar and lunisolar calendars try to approximate.

A mean tropical year is an average over a very long period of time (such as a 25800-year precession cycle). However, there are many types of mean tropical year. Normally a tropical year is measured from one solstice or equinox to the next. However, this presents two accuracy problems:

Length of Time Between Successive March Equinoxes
(from [150], page 41)

1985-86 365d 5h 48m 58s = 31556938 sec
1986-87 365d 5h 49m 15s = 31556955 sec (+17)
1987-88 365d 5h 46m 38s = 31556798 sec (-140)
1988-89 365d 5h 49m 42s = 31556982 sec (+44)
1989-90 365d 5h 51m 6s = 31557066 sec (+128)

Mean Tropical Years Between Each Pair of Solstice or Equinox Type
(for the year 2000, from [150], page 42)
The "days" here are 1900 mean solar days ("ephemeris days")

Between two March equinoxes 365.242374 days
Between two June solstices 365.241626 days
Between two September equinoxes 365.242018 days
Between two December solstices 365.242740 days
Laskar's mean tropical year
(average over the whole orbit)
365.242189 days

On geologic timescales the Earth's rotational period (length of the solar day) increases by about 2.3 milliseconds per day per century. Longer days means fewer days per year, so the length of the tropical year decreases every year by about 2.7×10-10 days. This is mainly due to the tidal interaction with the Moon126 slowing Earth's rotation (see 9192631770 for more about this). In addition, there is an effect called post-glacial rebound that operates on shorter timescales (the period since the last ice age) causing the Earth's rotation to speed up by about 0.7 milliseconds per day per century, making the tropical year increase by 8.1×10-11 days per year. This adds to the lunar effect, making for an overall increase of the day length of +1.7 milliseconds per century, and an overall decrease of the number of solar days per tropical year of 1.96×10-10 every year.

There are also shorter-term variations that fluctuate so much that it doesn't even make sense to try to average them into a year length figure; see mean solar day.

The following numbers, close to 365.242, are approximations to the tropical year; compare to the sidereal year constants which are higher.


365.242189670

One value of the tropical year in mean solar days. This figure was in the Wikipedia Year article in 2008; later shortened to "365.24219". Both are intended to be for the year 2000. The mean solar day and other factors vary too much to get more than about 9 digits of accuracy; see that entry and the tropical year article for details.

365.242190402

The length of the mean tropical year in "SI days" of 86400 SI seconds, for the year 2000 based on [152] ("The constants P1 and e0", p. 664 and "Mean elements of the Earth", p. 675):

365.25×1000 × 360×60×60 / (1295977422.83429 + 50288.200) = 365.242190402

This calculation is derived the same way as that for the sidereal year value 365.256363004 (see that entry for details), but adding Simon's rate of movement of the solstices, 50288.200 arc-seconds per millennium.

This number differs from other values of the tropical year for reasons discussed under tropical year and mean solar day.

365.242198781

Length of the tropical year, in "SI days" of 86400 SI seconds, by the "Besselian year" definition; see also 2415020.31352.

365.24220305...

The approximation to the tropical year known to the Mayan/mesoamerican people, who knew that 29 calendar rounds was very nearly equal to 1507 tropical years. See 550420.

365.242222222..

Length of the tropical year (in mean solar days) under the "Revised Julian calendar" of the Eastern Orthodox Church. In it, years divisible by 4 are leap years, except that years divisible by 100 are only leap years if dividing the year by 900 leaves a remainder of 200 or 600. This gives the approximation 365 + 1/4 - 1/100 + 2/900 = 365.242222222..

365.242374

An approximation to the tropical year from measuring between vernal equinoxes. As of 2012, this is given in the Wikipedia article Leap year, calling it the "vernal equinox year" (earlier versions gave 365.242375).

The length of time from one equinox to the next of the same type is not exactly the same as the tropical year, because the Earth's axial precession (see 25772.1300) moves at a different rate from the precession of the perihelion of the Earth's orbit (see anomalistic year). In modern times the Earth is furthest from the Sun (and thus moves slowest) in early July.

365.242375

An approximation to the tropical year from measuring between vernal equinoxes. This is seen in some discussions, most getting the number from Wikipedia Leap year, which cited this value as the "vernal equinox year"; later it switched to 365.242374.

365.2425

(the Gregorian year)

This is the approximation that the Gregorian calendar uses for the number of days in a tropical year. Note the series of approximations:

365, the Egyptian civil year
365 + 1/4 = 365.25, the Julian year
365 + 1/4 - 1/100 = 365.24, a slightly better approximation (but not used in any calendar)
365 + 1/4 - 1/100 + 2/900 = 365.242222222.., the revised Julian calendar year
365 + 1/4 - 1/100 + 1/400 = 365.2425, the Gregorian year

365.2468

This is the approximation that the Hebrew lunisolar calendar uses for the number of days in a tropical year.

365.25

(the Julian year)

The Julian year was the length (in days, or more accurately mean solar days) of the tropical year under the Julian calendar.

This approximation was probably first known to the Egyptians, who used a civil calendar of 365-day years (with no leap-years) for a staggeringly long period of time, and were therefore able to measure how inaccurate it was through observation of star risings (effectively measuring the difference between their 365-day civil year and the sidereal year). The discrepancy between this and the more accurate modern values of the tropical year results from the Egyptians' use of Sirius, a star far from the Ecliptic, to determine the length of a sidereal year and assuming that the tropical and sidereal years were the same. See the Sothic cycle and 1508.0833.

The Coptic calendar and Ethiopian calendar still use this approximation, because they have a leap year every 4 years without exception. There is further discussion of this and the Maya calendar (also still in use) in the entry for 365.


The Sidereal Year

A sidereal year is the amount of time it takes Earth to complete one orbit around the Sun when viewed from a nonrotating reference frame (which is usually approximated by averaging together the positions of many distant stars). It differs from the tropical year because of the Earth's axial precession.

There are different values for the sidereal year because the rate of Earth's rotation changes over time, and it has been measured in different ways; see the tropical year and mean solar day entries for details.

The following numbers, close to 365.256, are approximations to the sidereal year; compare to the tropical year constants which are lower.


365.25636042

Simon Newcomb's value for the length of a sidereal year in mean solar days. In Newcomb's work it appears as a parametrized formula:

t = 365.25636042 + 0.00000011T

where T is the number of centuries that have elapsed since 1900. Thus, for the year 2012, the sidereal year would be about 365.25636054 mean solar days.

See also 365.2568983.

365.256363004

Length of the sidereal year in "SI days" of 86400 SI seconds, for the year 2000 based on [152] ("Mean elements of the Earth", page 675). It gives the rate of Earth's motion around its orbit as 1295977422.83429 arc-seconds per 1000 Julian years. A Julian year is 365.25×86400 SI seconds, so the rate of movement would be

R = 1295977422.83429 / 1000×365.25×86400 ≈ 0.0410670463797

arc-seconds per SI second. The number of arc-seconds in a full circle is 360×60×60, so the length of the sidereal year in "SI days" would be:

Ys = 360×60×60 / 86400 R

To compute directly from the original number:

365.25×1000 × 360×60×60 / 1295977422.83429 = 365.256363004

This number differs from other values of the tropical year for reasons discussed under tropical year and mean solar day.

See also 365.242190402 and 365.2568983.

365.2563835

An approximate value of the sidereal year used in Carl Friedrich Gauss' Theoria Motus, and cited by [133]. See also 365.2568983.

365.2568983

(Gauss' sidereal year)

The value of the sidereal year corresponding to the following definition of the astronomical unit:

[An Astronomical Unit is] the radius of an unperturbed circular orbit a massless body would revolve about the sun in 2π/k days (i.e., 365.2568983.... days), where k is defined as the Gaussian constant exactly equal to 0.01720209895.

See also 365.256363004 and 365.2563835.

365.259636

(the anomalistic year)

An approximate value (for the year 2011) of the number of days between successive passages of the Earth through its Perihelion. This is the longest version of the "length of a year".

When viewed from the north ecliptical pole in a non-rotating position (i.e. "from the fixed stars"), the ellipse of the Earth's orbit moves "counter-clockwise" making one full turn in about 112,000 years. This is Apsidal precession; most of this effect comes from Earth getting "pulled forward" by Jupiter while it orbits the Sun.

Meanwhile, the direction of the Earth's rotational axis moves "clockwise", making a cycle in about 25,800 years. Since the Earth itself moves "counter-clockwise" in its orbit, the tropical year is shorter than the sidereal year, while the anomalistic year is longer.

366

Number of days in a leap year. See 365 and 365.25 for a discussion of 365-day calendars that are still in use.

368

A reader asked (roughly) the following:

What are the odds of seeing the digits 3, 6 and 8 (in any order, but contiguous) on an automobile license plate? If I see 1000 plates during my drive to work, it is unusual to see 10 cars that feature one of the combinations 368, 386, 638, 683, 836 or 863?

Of course, the answer depends a lot on how many license plates have digits at all, and whether there are lots of plates with 4 or more digits in them, etc. You have to consider how many cars there are with each different number of digits, and figure the odds for each.

For plates with 3-digit numbers, the answer is easy: 6 out of 1000. If all the plates had 3-digit numbers, then seeing 10 out of 1000 would be a bit higher than expected, but not much.

In general, the odds of seeing your N special digits in an N-digit number are N!/10N. (This is assuming the special digits are different from each other. If some of them are the same, the odds go down.)

For plates with more than N digits, the odds are a little more complicated to compute. For example, for 3 digits in a 4-digit number, the odds are 114 out of 10000. This is 6 less than 120/10000, which is what you get if you take the 6/1000 odds for the 3-digit case and double it. The reason is that you get:

- 60 cases with the 3 digits at the beginning of the 4-digit number

- 60 cases with the 3 digits at the end

- minus 6 cases that got counted twice because the first three are a match and the last three are also a match. These are the 6 cases that consist entirely of the 3 special digits, and have the first and last digit the same: 3683, 3863, 6386, 6836, 8368 and 8638.

114 out of 10000 is equivalent to 11.4 out of 1000. So if all the plates had 4-digit numbers, seeing 10 out of 1000 on your way to work is just about what you'd expect.

The general formula for the N+1 case is (2×10-1)N!/10(N+1)

As you would expect, the formula keeps getting more complicated. For the N+2 case it's ((3×10-2)×10-1)N!/10(N+2). So the odds of seeing 368, 386, etc. in 5-digit license plate numbers is 1674 out of 100000, or 16.74 out of 1000.

See also 0.543643....


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Quick index: if you're looking for a specific number, start with whichever of these is closest:    0.065988...    1    1.618033...    3.141592...    4    12    16    21    24    29    39    46    52    64    68    89    107    137.03599...    158    231    256    365    616    714    1024    1729    4181    10080    45360    262144    1969920    73939133    4294967297    5×1011    1018    5.4×1027    1040    5.21...×1078    1.29...×10865    1040000    109152051    101036    101010100    — —    footnotes    Also, check out my large numbers and integer sequences pages.


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