exoplanet discovery archive · 1992 – 2017

A scrollable history of every
world we’ve almost seen.

Scroll the lens through two and a half decades of discovery. Each dot is a confirmed exoplanet, plotted by orbital period and radius. Planets we’ve seen clearly hold still. Planets with missing data flicker, we know they’re there, but we don’t have all their data.

// about the dataset

This catalog draws from a comprehensive archive of 3,500+ exoplanets with discoveries from 1992 to 2017. Each entry records orbital mechanics, planetary size, host star properties, discovery method, and surface temperature where known.

// how to read the lens

Each dot is a confirmed exoplanet, plotted by orbital period and radius. Planets we’ve seen clearly hold still. Planets with missing data flicker, we know they exist, but their full story is unwritten. Hover any dot to inspect it.

// how to read the timeline

Next to thelens sits a scrollable discovery timeline. Drag up or down to move through years. The lens will react to the timeline scrolling and show you the planets based on the discovery year selected.

Scroll1992 → 2017
Start
Planets showing until 1992 0 in view
All planets up to this year
Show Solar System
Discovery methods [ Show All ]
Transit Radial velocity Imaging Microlensing Timing Other
Flickering dots are planets with missing data.
● Size: Planet Radius
● Opacity: Distance (further = fainter)
FIG · AAnnual yield · 1992–2017

Discoveries per year

Transit RV Others
FIG · BFor this year’s batch

Data completeness

SUMMARIZED UNTILNote
1781
Loading…
This year · 0
Running total · 0
Method mix ·
Panel 01Scatter · log–lin

Hot Jupiters cluster around metal‑rich suns.

Giant gas planets orbiting extremely close to their stars, known as "Hot Jupiters", are far more common around stars with high metal content (metallicity). This provides strong evidence for the core accretion model of planet formation, where heavy elements are needed to rapidly build planet cores before the stellar gas dissipates.

Transit Radial velocity Imaging Microlensing Timing Other
[ Show All ] [ Click to filter ]
Panel 02Bubble · log–log

What if someone else wanted to look for us?

All confirmed exoplanets are plotted by discovery method, with our own Solar System planets highlighted in white. If an alien civilization used our current technology to look at our Solar System, they would not be able to detect Earth. Our home planet is too small and too far from the Sun to be seen with our current instruments—meaning the universe could be full of Earths that remain invisible to us.

Only planets with a measured radius are shown, radius requires a transit, so this view is intrinsically transit-heavy.

Transit Radial velocity Imaging Microlensing Timing Other Solar System
[ Show All ] [ Click to filter ]
Panel 03Coverage · 25 fields

The columns we leave blank.

This chart shows the fill rate across 25 different planetary and stellar attributes in the catalog. While basic metadata like the discovery year and method are 100% complete, critical physical properties quickly thin out. Highlighted in red are parameters with critical data gaps (under 50% completeness)—such as the planet's age (ageGyr), which is recorded for less than 1% of all discovered worlds.

Twenty‑five years. Three thousand five hundred worlds. And still, the most honest chart in this story is the one full of empty columns. Every gap is a planet half‑known, a mass without an age, an orbit without a temperature. The history of exoplanet discovery isn’t finished. It’s barely been started.