TOI-672 b
{{Short description|Neptune-like exoplanet}}
{{Infobox planet
| extrasolarplanet = yes
| name = TOI-672 b
| image =
| image_size =
| image_alt =
| caption =
| apsis =
| discoverer =
| discovery_site =
| discovered = 2023
| discovery_method = Transit
| alt_names =
| periastron =
| apoastron =
| semimajor =
| avg_speed =
| eccentricity = 0.0
| period = 3.6 days
| synodic_period =
| inclination = {{val|88.43|0.82|ul=Degree (angle)}}
| angular_dist =
| long_periastron =
| time_periastron =
| semi-amplitude =
| star = TOI-672
| mean_radius = {{val|0.470|0.008|0.009|ul=Jupiter radius}}
| surface_area =
| volume =
| density =
| mass = {{val|0.0760|ul=Jupiter mass}}
| surface_grav =
| moment_of_inertia_factor =
| escape_velocity =
| albedo =
| single_temperature = 676.15 K
}}
TOI-672 b is a Neptune-like exoplanet, located 218 light-years away. The exoplanet was discovered in the year 2023.
Characteristics
= Mass and radius =
TOI-672 b was discovered by the transit method. Its mass is {{val|0.0760|ul=Jupiter mass}} or {{val|24.1|ul=Earth mass}}. The exoplanet currently has a radius of {{val|0.470|0.008|0.009|ul=Jupiter radius}} or {{val|5.26|0.08|0.10|ul=Earth radius}}.
= Orbit =
TOI-672 b has a smaller orbital period than Mercury. The exoplanet has an orbital period of 3.6 days, just like Kepler-444 b and has an inclination of {{val|8.43|0.82|ul=Degree (angle)}}.
Host star
The host star of the exoplanet is TOI-672.
The host star is a M-type star and is not visible to the naked eye from Earth. The star has a mass of {{val|0.54|0.02|ul=Solar mass}}, a radius of {{val|0.544|0.0163|ul=Solar radius}} and a temperature of {{val|3765|65|ul=Kelvin}}.