Exoplanets · Constellation Aquarius

TRAPPIST-1 e

Coordinates, Gaia distance (12.47 pc), 6.10-day orbital period, mass 0.692 M⊕, radius 0.920 R⊕, and JWST transit spectroscopy for TRAPPIST-1 e.

Right Ascension (J2000.0)23h 06m 29.28s
Declination (J2000.0)-05° 02′ 28.6″
Primary ClassificationTemperate terrestrial exoplanet in a 7-planet resonant chain
Best Observing SeasonLate Summer to Autumn (August–November)

Provenance-Backed Scientific Measurements

Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.

Astrometric, Photometric, and Physical Parameters for TRAPPIST-1 e
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Orbital period6.099615 d± 0.000011 dMulti-telescope transit timing (Spitzer/Kepler/HST/JWST)definitiveNASA Exoplanet Archive
Planetary radius0.92 R⊕± 0.013 R⊕Transit photometry (R_p / R_★ = 0.0689)definitiveNASA Exoplanet Archive
Planetary mass0.692 M⊕± 0.022 M⊕7-planet resonant transit-timing variations (Agol et al. 2021)definitiveNASA Exoplanet Archive
Orbital semi-major axis0.02925 AU± 0.00025 AUKeplerian dynamical solution around 0.0898 M☉ host stardefinitiveNASA Exoplanet Archive
Zero-albedo equilibrium temperature251.3 K± 4.9 KDerived from 0.662 S⊕ stellar insolationmodel-dependentNASA Exoplanet Archive
Host star distance (Gaia DR3)12.467 pc± 0.006 pcGaia DR3 astrometric parallax (80.21 ± 0.04 mas, 40.66 ly) (J2016.0)definitiveESA Gaia Archive — Data Release 3
Measurement Uncertainties & Competing Solutions: Transit-timing variations (TTVs) among the seven resonant TRAPPIST-1 planets determine TRAPPIST-1 e's mass (0.692 ± 0.022 M⊕) and bulk density (0.889 ± 0.033 ρ⊕) to ~3%, though JWST NIRSpec transmission spectra continue to face stellar-spot contamination ('the transit light-source effect') when probing for a secondary N2/CO2 atmosphere.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots TRAPPIST-1 e (Temperate Terrestrial World) at RA 23h 06m 29.28s, Dec -05° 02′ 28.6″ within Aquarius, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.

J2000 Equatorial Sky Position (Aquarius) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 45° 40°N Lat 65° 30°S Lat RA: 23h 06m 29.28s Dec: -05° 02′ 28.6″ Epoch: J2000.0 First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

TRAPPIST-1 e is the fourth planet from the ultracool M8 V dwarf star TRAPPIST-1, located 12.467 ± 0.006 parsecs (40.66 light-years) away in Aquarius. Discovered in 2017 using the Transiting Planets and Planetesimals Small Telescope (TRAPPIST) and NASA's Spitzer Space Telescope, TRAPPIST-1 e orbits inside a compact Laplace mean-motion resonant chain of seven Earth-sized worlds, all packed closer to their miniature 2,566 K red-dwarf sun than Mercury is to ours.

Completing one orbit every 6.0996 days at a distance of just 0.02925 AU (4.38 million kilometers), TRAPPIST-1 e receives 66.2% of Earth's solar flux, placing it squarely in the conservative liquid-water habitable zone with a zero-albedo equilibrium temperature of 251 K (−22 °C). Because the seven planets gravitationally tug on one another at every conjunction, their transit times shift by minutes to hours; inverting those transit-timing variations yields a rocky, iron-core bulk density of 4.89 g/cm³ (0.692 Earth masses inside 0.920 Earth radii)—the closest known analog to Earth's uncompressed interior composition.

Because TRAPPIST-1 has a radius only 11.9% that of the Sun (slightly larger than Jupiter), TRAPPIST-1 e blocks 0.475% (4,750 ppm) of the star's light during every 57-minute transit—nearly 56 times deeper than an Earth-across-the-Sun transit—making it the premier terrestrial target for atmospheric transmission spectroscopy with the James Webb Space Telescope.

Practical Visual Observing Guide

Minimum Instrument250–350 mm telescope + near-IR/CMOS camera (V = 18.80, J = 11.35)
Recommended MagnificationAstrophotometry / NIR transit light-curve target
Best Evening SeasonLate Summer to Autumn (August–November)
  • The host star TRAPPIST-1 is an ultra-faint M8 V red dwarf shining at visual magnitude V = 18.80 (though much brighter in the near-infrared at J = 11.35 and K = 10.30).
  • Visual observation of the host star requires a 500 mm (20-inch) or larger telescope under dark skies, while amateur CCD/CMOS observers with 250–350 mm telescopes equipped with near-IR/I-band filters can record the star's 11.3-mag infrared flux and detect the 0.005-magnitude transit dip.

Catalog Cross-Identifications & Aliases

Common Aliases: 2MASS J23062928-0502285 e

Cross-Catalog Identifiers for TRAPPIST-1 e
Catalog AuthorityIdentifier
NASAEXOPLANETTRAPPIST-1 e
SIMBADTRAPPIST-1 e
WIKIDATAQ28822650
Related Object · Centaurus

Proxima Centauri b (Nearest Exoplanet)

Coordinates, ESPRESSO minimum mass (1.07 M⊕), 11.186-day habitable-zone orbit at 0.04856 AU, and stellar flare environment of Proxima Centauri b.

Related Object · Leo

K2-18 b (Temperate Sub-Neptune in Leo)

Coordinates, Gaia DR3 distance (38.07 pc), 32.94-day habitable-zone orbit, 8.63 M⊕ mass, 2.61 R⊕ radius, and JWST CH4/CO2 spectrum of K2-18 b.

Related Object · Pegasus

51 Pegasi b (Dimidium First Hot Jupiter)

Coordinates, Gaia DR3 distance (15.46 pc), 4.2308-day orbital period, Nobel-winning radial-velocity discovery, and observing guide for 51 Pegasi b.

Reference Guide

Trigonometric Parallax, Parsecs & Gaia DR3

How trigonometric parallax (d_pc = 1 / p_arcsec), the distance modulus equation, Hipparcos, and Gaia DR3 microarcsecond astrometry measure cosmic distances.

Catalog · NASA Exoplanet Archive (NExScI)

Confirmed Exoplanets & Host Systems Catalog

Curated NASA Exoplanet Archive reference catalog of benchmark exoplanets: Proxima Centauri b, TRAPPIST-1 e, 51 Pegasi b, HD 209458 b, K2-18 b, and WASP-39 b.

Scientific Sources & Dataset Provenance

  • NASA Exoplanet Archive (2026-10-01 snapshot): Akeson, R. L., et al. 2013, PASP, 125, 989; NASA Exoplanet Archive (IPAC/Caltech) — NASA Exoplanet Science Institute (NExScI / Caltech / IPAC)
  • JWST / MAST Science Archive & Mission Documentation (Cycle 1–4 Public Releases (2022–2026)): Rigby, J., et al. 2023, PASP, 135, 048001 (The Science Performance of JWST as Characterized in Commissioning) — NASA / ESA / CSA / STScI
  • ESA Gaia Archive — Data Release 3 (DR3 (2022-06-13)): Gaia Collaboration, Vallenari, A., et al. 2023, A&A, 674, A1 (Gaia Data Release 3) — European Space Agency / Gaia DPAC