Kepler-298d
{{Short description|Exoplanet in the habitable zone}}
{{Infobox planet
| name = Kepler-298d
| discovery_site = Kepler
| discovered = February 26, 2014
| discovery_method = Transit method
| apsis = astron
| time_periastron = JD 2454985.64156
| star = Kepler-298
| mean_radius = 2.50 ± 0.20 {{Earth radius|link=y}}
| density = {{convert|2.8203|±|4.0164|g/cm3|lk=on|abbr=on}}
}}
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.{{cite encyclopedia|url=https://exoplanet.eu/catalog/kepler_298_d--1890/|encyclopedia=Extrasolar Planets Encyclopaedia|title=Planet Kepler-298 d|access-date=26 April 2018}} The planet was originally considered to be potentially habitable,{{cite journal |last1=Safonova |first1=M. |last2=Murthy |first2=J. |last3=Shchekinov |first3=Yu. A. |title=Age aspects of habitability |journal=International Journal of Astrobiology |date=27 August 2018 |volume=15 |issue=2 |page=10 |doi=10.1017/S1473550415000208 |arxiv=1404.0641 }} but further research places its atmosphere at +2.11 on the HZA scale,{{technical inline|date=January 2025}} meaning it may be an ocean planet with a thick gas atmosphere like a gas dwarf.{{Cn|date=December 2023}}