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| mass = {{nowrap|1.18 ± 0.12<ref name="Borgniet2017"/>}} ...irginis is an [[F-type main sequence star]] that is approximately 118% the mass of and 145% the radius of the [[Sun]]. It has a temperature of 6557 [[Kelvi ...

| mass = {{val|0.118|0.002}} ...ed by the [[Transiting Exoplanet Survey Satellite]].<ref>{{Cite web |title=Planetary Systems |url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph- ...

...ant impacts phase, characterized by significant collisions between forming planetary bodies. These impacts play a pivotal role in shaping the structure, composi ...ing that substantial collisions between protoplanets could explain various planetary characteristics. Key milestones in this research include the formulation of ...

{{short description|Old star with a planetary system}} | mass = {{val|0.902|0.040|0.038}}<ref name="Saad-Olivera2017"/> ...

...'' ('''ESI''') is a proposed characterization of how similar a [[planetary-mass object]] or [[natural satellite]] is to [[Earth]]. It was designed to be a The scale has no quantitative meaning for [[Planetary habitability|habitability]]. ...

| mass = 1.05<ref name=starhorse/> ==Possible planetary system== ...

...he asteroid's path, and that neither the vehicle nor its expelled reaction mass come in direct contact with the asteroid. The tractor spacecraft could eit ...flection would require the determination of the asteroid's exact center of mass, and considerable effort might be necessary to halt its spin or rotation, b ...

| mass = {{Val|5.0|0.8}} ...of the Sun]].<ref name=lang2006/> It has five times the [[solar mass|Sun's mass]], and radiates 1,175 times the [[solar luminosity]] from its [[stellar atm ...

| mass = {{val|13.47|5.67|ul=Jupiter mass}}<ref name="Phillips2024"/> ...cility|NASA IRTF]] confirmed the presence of a young star with a planetary-mass companion around BD+60 1417.<ref name="Faherty2021" /> ...

...m]]<ref>{{Cite web|url=https://sphere.osug.fr/spip.php?rubrique7|title=Odd planetary system around fast-spinning star doesn't quite fit existing models of plane | mass = {{val|7.1|1.2|ul=Jupiter mass}}<ref name="Carter et al" /> ...

| mass = {{val|1.243|0.054}}<ref name=Muterspaugh2010/> ...e system in 1996.<ref>{{cite journal|last=Benest|first=D.|date=1996|title= Planetary orbits in the elliptic restricted problem. III. The η Coronae Borealis syst ...

| mass = 0.61 ± 0.03<ref name="Keplercitepaper"/> ...], although other phenomenon can also be responsible which is why the term planetary candidate is used.<ref name = "Morton">{{Cite journal | last1=Morton | firs ...

...sulting in smaller terrestrial planets, a small mass of [[Mars]] and a low mass asteroid belt. ...pressure supported and as a result orbits at a velocity slower than large objects.<ref name=Kretke_2014 /> The gas affects the motions of the solids in varyi ...

| mass = {{Val|5.9|0.2}}<ref name=Tetzlaff2011/> ...has an estimated 5.9<ref name=Tetzlaff2011/> times the [[solar mass|Sun's mass]] and radiates 1,291<ref name=Mcdonald2012/> times the [[solar luminosity]] ...

{{short description|Lowest possible mass of the celestial object}} ...line-of-sight; Doppler spectroscopy will give a true value of the planet's mass.<br />''Right'': In this case none of the star's movement is along the view ...

...net-discovered-neutron-star.html |access-date=August 25, 2011}}</ref> <!--Mass (in solar masses)--> ...-1438|period_unit=hour}}{{Orbitbox planet|exoplanet=[[PSR J1719-1438 b|b]]|mass=~1.02|mass_earth=|semimajor=0.004|period=2.176951032|eccentricity=<0.06|rad ...

| mass = 0.453{{±|0.002}}<ref name=Rattanamala2021/> ...former is 18% as massive as the Sun, while the latter has 44% of the Sun's mass.<ref name="Bruch">{{Cite journal | last1 = Bruch | first1 = A. | last2 = Di ...

...combined mass of the active stars in this cluster is about 630 times the [[mass of the Sun]].<ref name=aaa386/> ...into [[white dwarf]]s or other [[stellar remnant]]s. The remainder of lost mass consists of stars that have migrated away from the main body of the cluster ...

|mass = 1.83<ref name = Kervella2021/> ...un]]'s girth.<ref name = Kervella2021/> At present it has 1.83 times the [[mass of the Sun]]<ref name = Kervella2021/> and shines with a [[luminosity]] of ...

...{smallmatrix}\frac{4 \pi^2}{T^2} = \frac{G M}{R^3}\end{smallmatrix}</math> Mass and the period are known, so the equation can be written with semimajor axi | mass = ~2.7<ref name=PHL/> {{Earth mass|link=y}} ...