DEEP FIELDan atlas of the observable universe

01 · The neighborhood

A solar system that actually moves

Eight planets orbiting in real proportion — one Earth year passes every ten seconds. Orbits are spaced on a log scale so Mercury and Neptune fit in one frame. Click any planet.

t = 0.0 yr

Distance from Sun
Light travel time
Year length
Known moons

The fact sheet, sortable

Values from the NASA NSSDCA Planetary Fact Sheet — U.S. government data, public domain. Click a column to rank the planets by it.

Planet Mass
(10²⁴ kg)
Diameter
(km)
Density
(kg/m³)
Gravity
(m/s²)
Escape v
(km/s)
Day length
(hours)
Sun distance
(10⁶ km)
Orbit
(days)
Mean temp
(°C)
Moons
Mercury0.3304,8795,4293.74.34,222.657.988.01670
Venus4.8712,1045,2438.910.42,802.0108.2224.74640
Earth5.9712,7565,5149.811.224.0149.6365.2151
Mars0.6426,7923,9343.75.024.7228.0687.0−652
Jupiter1,898142,9841,32623.159.59.9778.54,331−11095
Saturn568120,5366879.035.510.71,432.010,747−140274
Uranus86.851,1181,2708.721.317.22,867.030,589−19528
Neptune10249,5281,63811.023.516.14,515.059,800−20016

Day lengths are the solar day; Saturn's density of 687 kg/m³ means it would float, if you could find the bathtub. Moon counts move as surveys find more — Saturn jumped past Jupiter in 2023.

09 · The Moon

Everything we know about the Moon

The only other world humans have stood on — and the best-measured object in the sky. The panel below is computed live in your browser from orbital mathematics; no server involved.

The Moon tonight computing…
Illuminated

Fraction of the disc lit as seen from Earth, from the current phase angle.

Distance right now ≈

First-order estimate from the Moon's elliptical orbit — good to a fraction of a percent. Mean distance: 384,400 km.

Next full moon

Computed from the 29.53-day synodic cycle. Check any almanac against this — it should agree to within hours.

It was born in a collision

The leading, sample-backed account: about 4.5 billion years ago a Mars-sized body — named Theia — struck the young Earth, and the Moon condensed from the debris. Apollo rocks share Earth's oxygen-isotope fingerprint, which is why this theory won.

It is leaving — slowly

Laser pulses bounced off retroreflectors left by Apollo crews measure the distance to millimeters. Verdict: the Moon spirals outward about 3.8 cm per year, stealing angular momentum from Earth and lengthening our days.

We only see one face

Tidal forces locked its rotation to its orbit long ago. But it wobbles — librations let patient observers glimpse about 59% of the surface over time. No one saw the far side until a spacecraft flew around in 1959.

Its two faces differ

The near side is painted with dark volcanic plains — the maria. The far side is almost all bright, battered highlands with a thicker crust. Why the asymmetry exists is still an open research question.

There is water ice

Inside polar craters that never see sunlight, temperatures stay cold enough to trap ice for billions of years. NASA's LCROSS impact confirmed water there in 2009 — the resource anchoring plans to return, this time to the south pole.

It quakes

Seismometers deployed by Apollo crews recorded moonquakes for years: deep quakes flexed by Earth's tides, thermal cracking at sunrise, and rare shallow quakes strong enough to matter for future bases.

It holds no air worth breathing

Only a whisper-thin exosphere. With no blanket, the equator swings from roughly −170 °C at night to over 100 °C in daylight — one reason Apollo missions landed at lunar morning.

Twelve people, 382 kilograms

Between 1969 and 1972, twelve humans walked its surface and carried home 382 kg of rock and soil — samples still being opened and studied with instruments that didn't exist when they were collected.

Mosaic of the far side of the Moon from the Lunar Reconnaissance Orbiter
The face we never see — the far side, mosaicked by Lunar Reconnaissance Orbiter. Almost no maria. Credit: NASA/GSFC/ASU
GRAIL gravity map of the Moon
The Moon, weighed — the GRAIL twins mapped its gravity field by flying in formation; the map exposes buried craters and crust thickness. Credit: NASA/JPL-Caltech/MIT/GSFC
Apollo 17 astronaut Harrison Schmitt beside a large boulder
The last footsteps, so far — geologist Harrison Schmitt at a boulder in the Taurus-Littrow valley, Apollo 17, December 1972. Credit: NASA

15 · Solar weather

When the Sun throws things

Two kinds of eruption matter to us. A solar flare is a flash of radiation that reaches Earth in 8 minutes. A coronal mass ejection (CME) is a billion-ton cloud of magnetized plasma that takes one to three days to arrive — and when it hits, it squeezes Earth's magnetic field, paints the sky with aurora, and can push currents through power grids. The live Kp dial at the top of this page and the aurora panel on the observatory wall are this section's instruments.

ABarely measurable background flickers.
BSmall — no effect at Earth.
CCommon — minor radio effects at most.
MMedium — brief radio blackouts, aurora likely with a CME.
XExtreme — each step is 10× the last, and X-class keeps counting up.
A flare erupts, in extreme ultravioletSolar Dynamics Observatory · NASA/GSFC — material blasting off the limb of the Sun
The "Phoenix" prominence eruptionSDO, 2015 · NASA/GSFC — a filament of plasma many Earths long lifting off
1859

The Carrington Event

The strongest geomagnetic storm on record. Aurora were reported near the tropics, and telegraph lines sparked — some operators sent messages on the storm's induced current alone. The benchmark for what the Sun can do to a wired civilization.

1989

Québec goes dark

A CME-driven storm collapsed the Hydro-Québec power grid in about 90 seconds, leaving millions without electricity for nine hours — the event that made space weather an engineering discipline.

16 · The far suburbs

The Kuiper Belt & the Oort Cloud

The planets are not where the solar system ends. Beyond Neptune lie two vast reservoirs of leftover construction material — one we have photographed, and one so far away we have only ever seen its messengers. The strip below is drawn to a logarithmic scale; on a linear one, everything you've met on this page so far would fit inside the first pixel.

Sun Earth · 1 AU Neptune · 30 Heliopause · ~120 Voyager 1 · ~171 Kuiper Belt · 30–55 AU Oort Cloud · ~2,000–100,000 AU next star ≈ 268,000

Logarithmic scale · 1 AU = the Earth–Sun distance · drawn by this page from the distances themselves

The Kuiper Belt — photographed

A doughnut of icy bodies from about 30 to 55 AU, holding Pluto, Eris, Makemake, Haumea, and hundreds of thousands of smaller worlds — the source of short-period comets. New Horizons crossed it and in 2019 photographed Arrokoth, a gently fused two-lobed body 6.6 billion km out: the most distant world ever visited.

It is still being mapped: in its first year and a half of test data, the Rubin Observatory added roughly 380 new trans-Neptunian objects, including two on orbits stretching about a thousand AU from the Sun.

The Oort Cloud — inferred, never seen

Honesty first: no one has ever observed the Oort Cloud directly. Its existence is deduced from the long-period comets that fall in from every direction of the sky, pointing back to a spherical shell of trillions of icy bodies roughly 2,000 to 100,000 AU out — the true gravitational edge of the Sun's domain, reaching a substantial fraction of the way to the next star.

Its scale defeats even our fastest machines: Voyager 1, doing 17 km/s for five decades, would need about 300 more years to reach its inner edge — and tens of thousands to pass through. When comet Hale-Bopp lit up the sky in 1997, you were looking at an Oort Cloud resident on a rare visit downtown.

Pluto and Charon photographed in color by New Horizons
Kuiper Belt royalty — Pluto and Charon, the belt's most famous residents, by New Horizons. Credit: NASA/JHUAPL/SwRI
Artist's size comparison of large trans-Neptunian objects
The belt's big worlds, compared — an artist's size lineup of major trans-Neptunian objects. Credit: NASA (artist's concept)
Hubble Space Telescope images of comet Hale-Bopp
A messenger from the Oort Cloud — comet Hale-Bopp under Hubble's eye: the closest we get to seeing the cloud itself. Credit: NASA/ESA

17 · Near-Earth objects

The watch — who is tracking the rocks

More than 40,000 near-Earth asteroids are now catalogued, and the system that watches them is genuinely global: survey telescopes feed every sighting to the IAU's Minor Planet Center — the world's clearinghouse — while NASA's CNEOS and ESA's NEO Coordination Centre independently compute each orbit a century ahead. Two UN-endorsed bodies, IAWN and SMPAG, exist to coordinate warning and response between nations. And in 2022 the theory got its first field test: NASA's DART spacecraft rammed the moonlet Dimorphos and shortened its orbit by about half an hour — the first time humanity deliberately moved a celestial body. ESA's Hera probe is on its way there now to inspect the crater.

Known near-Earth asteroids40,000+
1 km+ class~870 · mostly found
140 m+ classOnly ~40% found so far
Non-zero century risk~2,000 tracked closely
Rubin's first haul11,000+ asteroids · 33 NEOs
The blind spotSunward — Chelyabinsk 2013 arrived unseen
ObjectClosest approachMiss distanceSpeed
2026 PB92026-Aug-204.4 lunar distances11.0 km/s
2026 PX2026-Aug-232.4 lunar distances6.8 km/s
2024 RV122026-Sep-095.6 lunar distances12.1 km/s
2018 SP22026-Sep-305.0 lunar distances14.3 km/s
2015 TS2382026-Oct-084.7 lunar distances15.8 km/s
2022 UP62026-Oct-152.6 lunar distances9.0 km/s

Upcoming close approaches within 10 lunar distances — snapshot queried from the NASA/JPL CNEOS close-approach database on August 19, 2026. None poses a threat; passes like these happen constantly. Live table at CNEOS below.

Galileo spacecraft views of asteroid Ida
What we're tracking — asteroid Ida, photographed by the Galileo spacecraft; a typical rocky wanderer, 56 km long. Credit: NASA/JPL
The OSIRIS-REx Bennu sample container arriving at NASA Goddard
We even brought a piece back — the OSIRIS-REx capsule delivering asteroid Bennu samples to NASA in 2023. Credit: NASA
The repositories — the open front doors of planetary defense:

CNEOS — NASA/JPL orbits, risk lists & the live close-approach table · Minor Planet Center — the world's official catalog · ESA NEOCC — Europe's independent risk list · IAWN — the UN-endorsed warning network · Eyes on Asteroids — fly the catalog in 3D · NASA Planetary Defense — the program itself · ATLAS — the last-alert survey scanning the whole sky nightly
Passing Earth todaySize (est.)Miss distanceSpeed
querying NASA NeoWs…

Fetching today's tracked close approaches…