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N-Body
This benchmark performs an N-body simulation of the Jovian planets. It is repeated ten times.

Results

The execution time is the user time added to the system time, as returned by the bash "time" command.

Python Perl Gambas Gambas + JIT
Execution time (s) 22.4 33.3 20.8 3.07
vs. Python 1 1.44 0.93 0.14
vs. Perl 0.69 1 0.65 0.09
vs. Gambas 1.07 1.55 1 0.62
vs. Gambas + JIT 7.30 10.85 6.78 1

Python source code

#!/usr/bin/python

# The Computer Language Benchmarks Game
# http://shootout.alioth.debian.org/
#
# originally by Kevin Carson
# modified by Tupteq, Fredrik Johansson, and Daniel Nanz
# modified by Maciej Fijalkowski
# 2to3

import sys

def combinations(l):
    result = []
    for x in range(len(l) - 1):
        ls = l[x+1:]
        for y in ls:
            result.append((l[x],y))
    return result

PI = 3.14159265358979323
SOLAR_MASS = 4 * PI * PI
DAYS_PER_YEAR = 365.24

BODIES = {
    'sun': ([0.0, 0.0, 0.0], [0.0, 0.0, 0.0], SOLAR_MASS),

    'jupiter': ([4.84143144246472090e+00,
                 -1.16032004402742839e+00,
                 -1.03622044471123109e-01],
                [1.66007664274403694e-03 * DAYS_PER_YEAR,
                 7.69901118419740425e-03 * DAYS_PER_YEAR,
                 -6.90460016972063023e-05 * DAYS_PER_YEAR],
                9.54791938424326609e-04 * SOLAR_MASS),

    'saturn': ([8.34336671824457987e+00,
                4.12479856412430479e+00,
                -4.03523417114321381e-01],
               [-2.76742510726862411e-03 * DAYS_PER_YEAR,
                4.99852801234917238e-03 * DAYS_PER_YEAR,
                2.30417297573763929e-05 * DAYS_PER_YEAR],
               2.85885980666130812e-04 * SOLAR_MASS),

    'uranus': ([1.28943695621391310e+01,
                -1.51111514016986312e+01,
                -2.23307578892655734e-01],
               [2.96460137564761618e-03 * DAYS_PER_YEAR,
                2.37847173959480950e-03 * DAYS_PER_YEAR,
                -2.96589568540237556e-05 * DAYS_PER_YEAR],
               4.36624404335156298e-05 * SOLAR_MASS),

    'neptune': ([1.53796971148509165e+01,
                 -2.59193146099879641e+01,
                 1.79258772950371181e-01],
                [2.68067772490389322e-03 * DAYS_PER_YEAR,
                 1.62824170038242295e-03 * DAYS_PER_YEAR,
                 -9.51592254519715870e-05 * DAYS_PER_YEAR],
                5.15138902046611451e-05 * SOLAR_MASS) }


SYSTEM = list(BODIES.values())
PAIRS = combinations(SYSTEM)


def advance(dt, bodies=SYSTEM, pairs=PAIRS):

    for (([x1, y1, z1], v1, m1),
	  ([x2, y2, z2], v2, m2)) in pairs:
	dx = x1 - x2
	dy = y1 - y2
	dz = z1 - z2
	mag = dt * ((dx * dx + dy * dy + dz * dz) ** (-1.5))
	b1m = m1 * mag
	b2m = m2 * mag
	v1[0] -= dx * b2m
	v1[1] -= dy * b2m
	v1[2] -= dz * b2m
	v2[0] += dx * b1m
	v2[1] += dy * b1m
	v2[2] += dz * b1m
    for (r, [vx, vy, vz], m) in bodies:
	r[0] += dt * vx
	r[1] += dt * vy
	r[2] += dt * vz


def report_energy(bodies=SYSTEM, pairs=PAIRS, e=0.0):

    for (((x1, y1, z1), v1, m1),
         ((x2, y2, z2), v2, m2)) in pairs:
        dx = x1 - x2
        dy = y1 - y2
        dz = z1 - z2
        e -= (m1 * m2) / ((dx * dx + dy * dy + dz * dz) ** 0.5)
    for (r, [vx, vy, vz], m) in bodies:
        e += m * (vx * vx + vy * vy + vz * vz) / 2.
    print("%.9f" % e)

def offset_momentum(ref, bodies=SYSTEM, px=0.0, py=0.0, pz=0.0):

    for (r, [vx, vy, vz], m) in bodies:
        px -= vx * m
        py -= vy * m
        pz -= vz * m
    (r, v, m) = ref
    v[0] = px / m
    v[1] = py / m
    v[2] = pz / m

def main():
    offset_momentum(BODIES['sun'])
    for t in range(10):
	report_energy()
	for n in range(100000):
	    advance(0.01)

    report_energy()

if __name__ == '__main__':
    main()

Perl source code

#!/usr/bin/perl -w

# The Computer Language Shootout
# http://shootout.alioth.debian.org/
#
# contributed by Christoph Bauer
# converted into Perl by Márton Papp
# fixed and cleaned up by Danny Sauer
# optimized by Jesse Millikan

use constant PI            => 3.141592653589793;
use constant SOLAR_MASS    => (4 * PI * PI);
use constant DAYS_PER_YEAR => 365.24;

#  Globals for arrays... Oh well.
#  Almost every iteration is a range, so I keep the last index rather than a count.
my (@xs, @ys, @zs, @vxs, @vys, @vzs, @mass, $last);

sub advance($)
{
  my ($dt) = @_;
  my ($mm, $mm2, $j, $dx, $dy, $dz, $distance, $mag);

#  This is faster in the outer loop...
  for (0..$last) {
#  But not in the inner loop. Strange.
    for ($j = $_ + 1; $j < $last + 1; $j++) {
      $dx = $xs[$_] - $xs[$j];
      $dy = $ys[$_] - $ys[$j];
      $dz = $zs[$_] - $zs[$j];
      $distance = sqrt($dx * $dx + $dy * $dy + $dz * $dz);
      $mag = $dt / ($distance * $distance * $distance);
      $mm = $mass[$_] * $mag;
      $mm2 = $mass[$j] * $mag;
      $vxs[$_] -= $dx * $mm2;
      $vxs[$j] += $dx * $mm;
      $vys[$_] -= $dy * $mm2;
      $vys[$j] += $dy * $mm;
      $vzs[$_] -= $dz * $mm2;
      $vzs[$j] += $dz * $mm;
    }

# We're done with planet $_ at this point
# This could be done in a seperate loop, but it's slower
    $xs[$_] += $dt * $vxs[$_];
    $ys[$_] += $dt * $vys[$_];
    $zs[$_] += $dt * $vzs[$_];
  }
}

sub energy
{
  my ($e, $i, $dx, $dy, $dz, $distance);

  $e = 0.0;
  for $i (0..$last) {
    $e += 0.5 * $mass[$i] *
          ($vxs[$i] * $vxs[$i] + $vys[$i] * $vys[$i] + $vzs[$i] * $vzs[$i]);
    for ($i + 1..$last) {
      $dx = $xs[$i] - $xs[$_];
      $dy = $ys[$i] - $ys[$_];
      $dz = $zs[$i] - $zs[$_];
      $distance = sqrt($dx * $dx + $dy * $dy + $dz * $dz);
      $e -= ($mass[$i] * $mass[$_]) / $distance;
    }
  }
  return $e;
}

sub offset_momentum
{
  my ($px, $py, $pz) = (0.0, 0.0, 0.0);

  for (0..$last) {
    $px += $vxs[$_] * $mass[$_];
    $py += $vys[$_] * $mass[$_];
    $pz += $vzs[$_] * $mass[$_];
  }
  $vxs[0] = - $px / SOLAR_MASS;
  $vys[0] = - $py / SOLAR_MASS;
  $vzs[0] = - $pz / SOLAR_MASS;
}

# @ns = ( sun, jupiter, saturn, uranus, neptune )
@xs = (0, 4.84143144246472090e+00, 8.34336671824457987e+00, 1.28943695621391310e+01, 1.53796971148509165e+01);
@ys = (0, -1.16032004402742839e+00, 4.12479856412430479e+00, -1.51111514016986312e+01, -2.59193146099879641e+01);
@zs = (0, -1.03622044471123109e-01, -4.03523417114321381e-01, -2.23307578892655734e-01, 1.79258772950371181e-01);
@vxs = map {$_ * DAYS_PER_YEAR}
  (0, 1.66007664274403694e-03, -2.76742510726862411e-03, 2.96460137564761618e-03, 2.68067772490389322e-03);
@vys = map {$_ * DAYS_PER_YEAR}
  (0, 7.69901118419740425e-03, 4.99852801234917238e-03, 2.37847173959480950e-03, 1.62824170038242295e-03);
@vzs = map {$_ * DAYS_PER_YEAR}
  (0, -6.90460016972063023e-05, 2.30417297573763929e-05, -2.96589568540237556e-05, -9.51592254519715870e-05);
@mass = map {$_ * SOLAR_MASS}
  (1, 9.54791938424326609e-04, 2.85885980666130812e-04, 4.36624404335156298e-05, 5.15138902046611451e-05);

$last = @xs - 1;

offset_momentum();

for (1..10)
{
  printf ("%.9f\n", energy());

  # This does not, in fact, consume N*4 bytes of memory
  for (1..100000){
    advance(0.01);
  }

}

printf ("%.9f\n", energy());

Gambas source code

#!/usr/bin/env gbs3

Class Body

  Static Private SOLAR_MASS As Float = 4 * Pi * Pi
  Private Const DAYS_PER_YEAR As Float = 365.24

  Public X As Float
  Public Y As Float
  Public Z As Float
  Public VX As Float
  Public VY As Float
  Public VZ As Float
  Public Mass As Float

  Static Public Sub Jupiter() As Body

    Dim P As New Body
    p.x = 4.84143144246472090e+00
    p.y = -1.16032004402742839e+00
    p.z = -1.03622044471123109e-01
    p.vx = 1.66007664274403694e-03 * DAYS_PER_YEAR
    p.vy = 7.69901118419740425e-03 * DAYS_PER_YEAR
    p.vz = -6.90460016972063023e-05 * DAYS_PER_YEAR
    p.mass = 9.54791938424326609e-04 * SOLAR_MASS
    return p

  End

  Static Public Sub Saturn() As Body

    Dim P As New Body
    p.x = 8.34336671824457987e+00
    p.y = 4.12479856412430479e+00
    p.z = -4.03523417114321381e-01
    p.vx = -2.76742510726862411e-03 * DAYS_PER_YEAR
    p.vy = 4.99852801234917238e-03 * DAYS_PER_YEAR
    p.vz = 2.30417297573763929e-05 * DAYS_PER_YEAR
    p.mass = 2.85885980666130812e-04 * SOLAR_MASS
    return p

  End

  Static Public Sub Uranus() As Body

    Dim P As New Body

    p.x = 1.28943695621391310e+01
    p.y = -1.51111514016986312e+01
    p.z = -2.23307578892655734e-01
    p.vx = 2.96460137564761618e-03 * DAYS_PER_YEAR
    p.vy = 2.37847173959480950e-03 * DAYS_PER_YEAR
    p.vz = -2.96589568540237556e-05 * DAYS_PER_YEAR
    p.mass = 4.36624404335156298e-05 * SOLAR_MASS
    return p

  End

  Static Public Sub Neptune() As Body

    Dim P As New Body

    p.x = 1.53796971148509165e+01
    p.y = -2.59193146099879641e+01
    p.z = 1.79258772950371181e-01
    p.vx = 2.68067772490389322e-03 * DAYS_PER_YEAR
    p.vy = 1.62824170038242295e-03 * DAYS_PER_YEAR
    p.vz = -9.51592254519715870e-05 * DAYS_PER_YEAR
    p.mass = 5.15138902046611451e-05 * SOLAR_MASS
    return p

  End

  Static Public Sub Sun() As Body

    Dim P As New Body

    p.mass = SOLAR_MASS
    return p

  End

  Public Sub OffsetMomentum(px As Float, py As Float, pz As Float) As Body

    vx = -px / SOLAR_MASS
    vy = -py / SOLAR_MASS
    vz = -pz / SOLAR_MASS

    Return Me

  End

End Class


Class NBodySystem

  Private Bodies As Body[]

  Public Sub _new()

    Dim PX, PY, PZ As Float
    Dim I As Integer

    Bodies = [ Body.Sun(), Body.Jupiter(), Body.Saturn(), Body.Uranus(), Body.Neptune() ]

    For I = 0 To Bodies.Max
      PX += Bodies[I].vx * Bodies[I].mass
      PY += Bodies[I].vy * Bodies[I].mass
      PZ += Bodies[I].vz * Bodies[I].mass
    Next

    Bodies[0].offsetMomentum(PX, PY, PZ)

  End

  Public Sub Advance(dt As Float)

    Dim I, J As Integer
    Dim iBody, jBody As Body
    Dim dx, dy, dz As Float
    Dim dSquared, fMag As Float
    Dim iMass, jMass, iMag, jMag As Float

    For I = 0 To Bodies.Max
      iBody = Bodies[I]
      iMass = iBody.mass

      For J = I + 1 To Bodies.Max
        jBody = Bodies[J]
	jMass = jBody.mass

        dx = iBody.x - jBody.x
        dy = iBody.y - jBody.y
        dz = iBody.z - jBody.z

        dSquared = dx * dx + dy * dy + dz * dz
        fMag = dt / (dSquared * Sqr(dSquared))
	iMag = iMass * fMag
	jMag = jMass * fMag

        iBody.vx -= dx * jMag
	iBody.vy -= dy * jMag
	iBody.vz -= dz * jMag

	jBody.vx += dx * iMag
	jBody.vy += dy * iMag
	jBody.vz += dz * iMag
      Next
    Next

    For Each iBody in Bodies
      iBody.x += dt * iBody.vx
      iBody.y += dt * iBody.vy
      iBody.z += dt * iBody.vz
    Next

  End

  Public Sub Energy() As Float

    Dim dx, dy, dz, distance, E As Float
    Dim iBody, jBody As Body
    Dim I, J As Integer

    For I = 0 To Bodies.Max

      iBody = bodies[i]
      E += 0.5 * iBody.mass * (iBody.vx * iBody.vx + iBody.vy * iBody.vy + iBody.vz * iBody.vz)

      For J = I + 1 To Bodies.Max

	jBody = Bodies[J]
        dx = iBody.x - jBody.x
        dy = iBody.y - jBody.y
        dz = iBody.z - jBody.z

        distance = Sqr(dx*dx + dy*dy + dz*dz)
        E -= (iBody.mass * jBody.mass) / distance

      Next
    Next

    return E

  End

End Class


Dim S As New NBodySystem
Dim I, N As Integer

For N = 1 To 10

  Print S.Energy()

  For I = 1 To 100000
    S.Advance(0.01)
  Next

Next

Print S.Energy()