Analysis of information sources in references of the Wikipedia article "Hill sphere" in English language version.
{{cite journal}}
: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link){{cite book}}
: CS1 maint: multiple names: authors list (link){{cite journal}}
: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link){{cite journal}}
: CS1 maint: multiple names: authors list (link) See also Hamilton, D.P. & Burns, J.A. (March 1991). "Orbital Stability Zones About Asteroids" (PDF). Icarus. 92 (1). New York, NY: Academic Press: 118–131. Bibcode:1991Icar...92..118H. doi:10.1016/0019-1035(91)90039-V. Retrieved 22 July 2023.{{cite journal}}
: CS1 maint: multiple names: authors list (link) cited therein.{{cite journal}}
: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link){{cite journal}}
: CS1 maint: multiple names: authors list (link) See also Hamilton, D.P. & Burns, J.A. (March 1991). "Orbital Stability Zones About Asteroids" (PDF). Icarus. 92 (1). New York, NY: Academic Press: 118–131. Bibcode:1991Icar...92..118H. doi:10.1016/0019-1035(91)90039-V. Retrieved 22 July 2023.{{cite journal}}
: CS1 maint: multiple names: authors list (link) cited therein.The moon's Hill sphere has a radius of 60,000 kilometres, about one-sixth of the distance between it and Earth.
{{cite journal}}
: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link){{cite journal}}
: CS1 maint: multiple names: authors list (link) See also Hamilton, D.P. & Burns, J.A. (March 1991). "Orbital Stability Zones About Asteroids" (PDF). Icarus. 92 (1). New York, NY: Academic Press: 118–131. Bibcode:1991Icar...92..118H. doi:10.1016/0019-1035(91)90039-V. Retrieved 22 July 2023.{{cite journal}}
: CS1 maint: multiple names: authors list (link) cited therein.