Space facts, computed today

29 facts, each one a sentence you can quote on its own. Every number was computed for at 18:00 UTC by the same engine behind our calculators and API, and the page is rebuilt by our daily almanac refresh.

On this page

Right now

Earth to Sun
149.1 million km
Age of sunlight
8 minutes 17 seconds
Earth to Moon
404,230 km
Moon illuminated
41 percent
Earth's orbital speed
29.89 km per second
Light time to Jupiter
47 minutes 28 seconds

Computed for 18:00 UTC on October 17, 2026. With JavaScript on, these six numbers update every second from your device clock; the numbered facts stay at the time above.

The sky behind these facts

The Moon, the planets and the stars the facts below keep naming, drawn by the renderer behind our Sky Map. It shows the sky over the city for your time zone (an approximation) and starts at tonight at 9 pm if the Sun is up. The buttons steer it; the numbered facts stay fixed at the time printed above.

Loads when you scroll to it. It needs JavaScript; the facts below do not.

Earth and the Sun

  1. On October 17, 2026, Earth is 149.1 million kilometers (0.9966 AU) from the Sun, 0.3 percent closer than the 149.6-million-kilometer average.

    Method: Heliocentric position of Earth from astronomy-engine (VSOP87 theory) at 18:00 UTC; 1 AU = 149,597,870.7 km (IAU 2012). The Earth

  2. The sunlight reaching Earth on October 17, 2026 left the Sun 8 minutes 17 seconds earlier.

    Method: The Earth-Sun distance in the fact above divided by the speed of light, 299,792.458 km/s. The Sun

  3. Earth's next perihelion is on January 3, 2027 at 02:08 UTC (in 78 days), when it will be 147.1 million kilometers from the Sun.

    Method: astronomy-engine SearchPlanetApsis for Earth, searched forward from 18:00 UTC on October 17, 2026. The anomalistic year

  4. On October 17, 2026, the Sun stands 9.5° south of the celestial equator and is drifting south by 0.36° per day.

    Method: Apparent declination of the Sun of date from astronomy-engine at 18:00 UTC; the daily drift is the change over the next 24 hours. The Sun's declination and the seasons

  5. On October 17, 2026, daylight at 40° N lasts 11 hours 5 minutes, 2 minutes 31 seconds shorter than the day before.

    Method: astronomy-engine sunrise and sunset (upper limb, standard refraction) at 40° N, 0° E for each UTC date; the length is sunset minus sunrise. Sunrise and sunset calculator

  6. On October 17, 2026, daylight at 40° N is 31 percent of the way from the December solstice length (9 hours 20 minutes) to the June solstice length (15 hours 1 minute).

    Method: Day length at 40° N from astronomy-engine for today and for the 2026 solstice dates; the percentage is (today - December) / (June - December). Equinoxes and solstices

  7. The next December solstice is on December 21, 2026 at 20:50 UTC (in 65 days).

    Method: astronomy-engine Seasons(): the instant the Sun's apparent ecliptic longitude reaches 0, 90, 180 or 270 degrees. December solstice

  8. On October 17, 2026, Earth is moving along its orbit at 29.89 kilometers per second (about 107,600 kilometers per hour), against an average of about 29.78.

    Method: Distance between astronomy-engine heliocentric positions of Earth one hour apart, centered on 18:00 UTC; the average is a circular orbit of 1 AU over one sidereal year. The Earth

  9. Since January 1, 2026 (00:00 UTC), Earth has traveled 743.3 million kilometers along its orbit, sweeping 284° as seen from the Sun, as of October 17, 2026.

    Method: Sum of hourly chords between astronomy-engine heliocentric positions of Earth from January 1 to 18:00 UTC on October 17, 2026; the sweep is the change in heliocentric ecliptic longitude. The Earth

  10. Since January 1, 2026 (00:00 UTC), Earth has rotated 290.54 times relative to the stars as of October 17, 2026, 0.79 more than the 289.75 solar days elapsed.

    Method: Elapsed time divided by the IERS mean sidereal day, 86,164.0905 s, against the 86,400 s solar day; the extra turns accumulate to one by the end of the year. Sidereal and solar day

The Moon

  1. At 18:00 UTC on October 17, 2026, the Moon is 404,230 kilometers from Earth, 5.2 percent farther than its 384,400-kilometer average distance.

    Method: Geocentric distance of the Moon from astronomy-engine, center to center, at 18:00 UTC. The Moon

  2. At 18:00 UTC on October 17, 2026, the light you see from the Moon left its surface 1.35 seconds earlier.

    Method: The Moon's distance in the fact above divided by the speed of light. The Moon

  3. The Moon's next perigee is on October 28, 2026 at 18:04 UTC (in 11 days) at 364,397 kilometers, and the next apogee follows on November 13, 2026 at 405,608 kilometers.

    Method: astronomy-engine SearchLunarApsis and NextLunarApsis, searched forward from 18:00 UTC on October 17, 2026. The anomalistic month

  4. At 18:00 UTC on October 17, 2026, the Moon is 41 percent illuminated and waxing, 7.1 days past new moon.

    Method: astronomy-engine illuminated fraction of the Moon's disc at 18:00 UTC; age is the time since the preceding new moon. Moon phase calendar

  5. The next full moon is on October 26, 2026 at 04:12 UTC (in 9 days), with the Moon 368,859 kilometers away.

    Method: astronomy-engine SearchMoonPhase for ecliptic longitude difference 180 degrees; distance is geocentric, at that instant. Full moon calendar

  6. The next new moon is on November 9, 2026 at 07:03 UTC (in 23 days).

    Method: astronomy-engine SearchMoonPhase for ecliptic longitude difference 0 degrees. Moon phase calendar

  7. The next full moon inside the 360,000-kilometer supermoon line is on December 24, 2026 (in 68 days), when the Moon will be 356,729 kilometers away.

    Method: astronomy-engine full moons from October 17, 2026, each tested against the 360,000 km line used on our supermoon page. Supermoons and micromoons

The planets

  1. On October 17, 2026, Mercury (24°) is in the evening sky, more than 15° east of the Sun (angle from the Sun in parentheses).

    Method: astronomy-engine Sun-planet elongation at 18:00 UTC; the 15 and 135 degree thresholds are the ones /v2/today uses. The label is sky-wide and ignores your horizon and latitude. Today in the sky

  2. On October 17, 2026, Mars (73°) and Jupiter (62°) are in the morning sky; Saturn (166°) is up most of the night; Venus (12°) is lost in the Sun's glare (angle from the Sun in parentheses).

    Method: astronomy-engine Sun-planet elongation at 18:00 UTC; the 15 and 135 degree thresholds are the ones /v2/today uses. The label is sky-wide and ignores your horizon and latitude. Today in the sky

  3. On October 17, 2026, Venus is 2 percent illuminated at magnitude -4.2, 12° from the Sun and 42.0 million kilometers from Earth.

    Method: astronomy-engine illuminated fraction, visual magnitude, Sun elongation and geocentric distance of Venus at 18:00 UTC. Venus tracker

  4. On October 17, 2026, Jupiter is 5.71 AU (853.7 million kilometers) from Earth, so its light takes 47 minutes 28 seconds to reach us.

    Method: Geocentric distance of Jupiter from astronomy-engine at 18:00 UTC, divided by the speed of light. Jupiter

  5. The next planet to reach opposition is Jupiter, on February 11, 2027 (in 117 days), when it will be 4.36 AU from Earth at magnitude -2.6.

    Method: astronomy-engine SearchRelativeLongitude for Mars, Jupiter and Saturn: the instant Earth and the planet share a heliocentric longitude, which is opposition. Earliest first; distance and magnitude at that instant. Jupiter

Eclipses and meteors

  1. The next eclipse is an annular solar eclipse on February 6, 2027 (in 112 days), with greatest eclipse at 16:00 UTC.

    Method: Our eclipse catalog (engine-computed, Saros series 131); date counted from October 17, 2026. Annular solar eclipse, February 6, 2027

  2. The most recent eclipse was a partial lunar eclipse on August 28, 2026, 50 days before October 17, 2026.

    Method: Our eclipse catalog (engine-computed, Saros series 138). Partial lunar eclipse, August 28, 2026

  3. The next total solar eclipse is on August 2, 2027, 289 days after October 17, 2026, in Saros series 136.

    Method: Our eclipse catalog (engine-computed); the day count is UTC calendar days from October 17, 2026. Total solar eclipse, August 2, 2027

  4. The next meteor shower to peak is the Orionids on October 21, 2026 at 18:09 UTC (in 4 days), rated at a zenithal hourly rate of 20, with the Moon 78 percent illuminated then.

    Method: Peak is the instant the Sun reaches the shower's solar longitude (astronomy-engine SearchSunLongitude); the rate is from the International Meteor Organization working list. Orionids

  5. The Geminids, listed at a zenithal hourly rate of 150, peak on December 14, 2026 (in 58 days), with the Moon 25 percent illuminated then.

    Method: Peak is the instant the Sun reaches the shower's solar longitude (astronomy-engine); the rate is from the International Meteor Organization working list. Geminids

The Sun's own cycle

  1. On October 17, 2026, Solar Cycle 25, which NOAA dates from December 2019, is 6.8 years old, about 62 percent of a nominal 11-year cycle.

    Method: Elapsed time since the cycle's start month in the NOAA SWPC record, over a nominal 11 years. An estimate: a cycle's length is only known after it ends. The sunspot cycle

  2. As of October 17, 2026, the latest monthly mean sunspot number in NOAA's record is 60.3, for September 2026, against 216.0 in August 2024, the highest month of Solar Cycle 25 so far.

    Method: NOAA Space Weather Prediction Center observed solar cycle indices (public domain), as stored in our sunspot index; refreshed monthly. The sunspot cycle

How these are computed

Positions come from astronomy-engine, the same build our API serves, so a fact here and the matching API answer cannot disagree. The eclipse dates come from our eclipse catalog, the meteor rates from the International Meteor Organization working list, and the sunspot numbers from NOAA's Space Weather Prediction Center. Each fact names its own method in the line beneath it.

Three conventions are worth knowing. Every time is UTC. Planets are sorted into evening sky, morning sky or lost in the Sun's glare by their angle from the Sun, a sky-wide label that does not account for your horizon or your latitude. Daylight is for 40° N, because day length depends on latitude and one number needs one latitude. Our methodology page covers accuracy and sources, and Today in the Sky turns the same engine toward your location.