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Kepler-298 d

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Kepler-298d is an exoplanet orbiting within the habitable zone of the orange dwarf star Kepler-298, located 1545 light years (473.69 parsecs) away from Earth. It was discovered in 2014 via the transit method. The planet was originally considered to be potentially habitable, but further research places its atmosphere at +2.11 on the HZA scale, meaning it may be an ocean planet with a thick gas atmosphere like a gas dwarf.

Astronomical data · SIMBAD

Object type
Pl
Distance
1,738 light-years
Coordinates
RA 283.0398° · Dec 48.8254°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Wikidata facts

Instance of
exoplanet
Constellation
Draco
Radius
0.223
Orbital period
77.473633
Show 12 more facts
located in/on physical feature
circumstellar habitable zone
discoverer or inventor
Kepler Space Telescope
right ascension
283.03980364581670
declination
48.82536562975778
epoch
J2000.0
time of discovery or invention
2014-03-00
discovery method
transit method
semi-major axis of an orbit
0.305
catalog code
TIC 48217868d
right ascension component of proper motion
6.295
declination component of proper motion
-8.198
parallax
1.9012

via Wikidata · CC0

~1 min read

Encyclopedic overview

2 sections
Contents
  • See also
  • References

Kepler-298d is an exoplanet orbiting within the habitable zone of the orange dwarf star Kepler-298, located 1545 light years (473.69 parsecs) away from Earth. It was discovered in 2014 via the transit method. The planet was originally considered to be potentially habitable, but further research places its atmosphere at +2.11 on the HZA scale, meaning it may be an ocean planet with a thick gas atmosphere like a gas dwarf.

==See also== List of potentially habitable exoplanets

Excerpted from Wikipedia’s “Kepler-298 d” article, available under the CC BY-SA 4.0 licence.