Apollo asteroid: Difference between revisions
Lede image consistent with Amor asteroid, Aten asteroid and Atira asteroid |
|||
(27 intermediate revisions by 20 users not shown) | |||
Line 1: | Line 1: | ||
{{Short description|Group of near-Earth asteroids}} |
|||
[[File:Minor Planets - Apollo.svg|thumb|285px|Location of the ''Apollo asteroids'' compared to the orbits of the [[terrestrial planet]]s of the [[Solar System]] |
|||
[[File:Neo orbit types.jpg|thumb|upright=2.4|Common orbital subgroups of [[Near-Earth Object]]s (NEOs)]] |
|||
{| style="width: 100%; margin-bottom: 8px; margin-left: 12px;" |
|||
⚫ | |||
| valign=top width=45% | |
|||
{{legend2|#e61d30|border=1px solid #770D18|[[Mars]]}} {{small|(M)}}<br /> |
|||
{{legend2|#000000|border=1px solid black|[[Venus]]}} {{small|(V)}}<br /> |
|||
{{legend2|#aaa|border=1px solid #444|[[Mercury (planet)|Mercury]]}} {{small|(H)}} |
|||
| valign=top | |
|||
{{legend2|#FFFF00|border=1px solid #B3B300|[[Sun]]}}<br /> |
|||
{{legend2|#00CC00|border=1px solid #003300|'''Apollo asteroids'''}}<br /> |
|||
{{legend2|#1708a6|border=1px solid black|[[Earth]]}} {{small|(E)}} |
|||
⚫ | |||
]] |
|||
The '''Apollo asteroids''' are a group of [[near-Earth asteroid]]s named after [[1862 Apollo]], discovered by German astronomer [[Karl Reinmuth]] in the 1930s. They are [[Earth-crosser asteroid|Earth-crossing asteroid]]s that have an orbital [[semimajor axis|semi-major axis]] greater than that of the Earth (> 1 [[Astronomical unit|AU]]) but [[perihelion]] distances less than the Earth's [[aphelion]] distance (q < 1.017 AU).<ref name="NEO-groups" /><ref name="Wolfram-Apollo" /> |
The '''Apollo asteroids''' are a group of [[near-Earth asteroid]]s named after [[1862 Apollo]], discovered by German astronomer [[Karl Reinmuth]] in the 1930s. They are [[Earth-crosser asteroid|Earth-crossing asteroid]]s that have an orbital [[semimajor axis|semi-major axis]] greater than that of the Earth (a > 1 [[Astronomical unit|AU]]) but [[perihelion]] distances less than the Earth's [[aphelion]] distance (q < 1.017 AU).<ref name="NEO-groups" /><ref name="Wolfram-Apollo" /> |
||
{{As of| |
{{As of|2024|10}}, the number of known Apollo asteroids is 20,412, making the class the largest group of [[near-Earth object]]s (''cf''. the [[Aten asteroid|Aten]], [[Amor asteroid|Amor]] and [[Atira asteroid|Atira]] asteroids),<ref name="neo-jpl-stats" /> of which 1,628 are [[Minor planet designation|numbered]] (asteroids are not numbered until they have been observed at two or more [[Opposition (planets)|oppositions]]), 79 are named, and 2,104 are identified as [[potentially hazardous asteroids]].<ref name="ssd-jpl">{{cite web |title=Small-Body Database Query |url=https://ssd.jpl.nasa.gov/tools/sbdb_query.html#!#results |website=Solar System Dynamics – Jet Propulsion Laboratory |publisher=NASA – California Institute of Technology |access-date=2024-10-11}}</ref><ref>{{cite web |title=List of Apollo Minor Planets |url=https://minorplanetcenter.net/iau/lists/Apollos.html |website=IAU Minor Planet Center |publisher=Center for Astrophysics |access-date=2024-10-11}}</ref> |
||
The closer their semi-major axis is to Earth's, the less [[Eccentricity (orbit)|eccentricity]] is needed for the [[orbit]]s to cross. The |
The closer their semi-major axis is to Earth's, the less [[Eccentricity (orbit)|eccentricity]] is needed for the [[orbit]]s to cross. The [[Chelyabinsk meteor]], that exploded over the city of [[Chelyabinsk#2013 meteor|Chelyabinsk]] in the southern Urals region of Russia on February 15, 2013, injuring an estimated 1,500 people with flying glass from broken windows, was an Apollo-class [[asteroid]].<ref name="USA-Today-Chelyabinsk" /><ref name="NewScientist-Chelyabinsk" /> |
||
== List == |
== List == |
||
Line 29: | Line 18: | ||
! Discoverer/First observed <sup>(A)</sup> |
! Discoverer/First observed <sup>(A)</sup> |
||
! Ref |
! Ref |
||
⚫ | |||
| {{mpl|2024 PT|5}} || align=center | 2024 || [[Asteroid Terrestrial-impact Last Alert System|ATLAS-SAAO]] || {{MPC|2024+PT5}} |
|||
⚫ | |||
|- |
|||
| {{mpl|2019 SU|3}} || align=center | 2019 || [[Asteroid Terrestrial-impact Last Alert System|ATLAS-HKO]] || {{MPC|2019+SU3}} |
|||
|- |
|- |
||
| {{mpl|2016 WF|9}} || align=center | 2016 || [[Wide-field Infrared Survey Explorer#NEOWISE (pre-hibernation)|NEOWISE]] || {{MPC|2016+WF9}} |
| {{mpl|2016 WF|9}} || align=center | 2016 || [[Wide-field Infrared Survey Explorer#NEOWISE (pre-hibernation)|NEOWISE]] || {{MPC|2016+WF9}} |
||
|- |
|- |
||
| {{mpl|2014 JO|25}} || align=center | 2014 || [[Catalina Sky Survey|CSS]] || {{MPC|2014+JO25}} |
| {{mpl|(671294) 2014 JO|25}} || align=center | 2014 || [[Catalina Sky Survey|CSS]] || {{MPC|2014+JO25}} |
||
|- |
|- |
||
| {{mpl|2013 FW|13}} || align=center | 2013 || CSS || {{MPC|2013+FW13}} |
| {{mpl|2013 FW|13}} || align=center | 2013 || CSS || {{MPC|2013+FW13}} |
||
|- |
|- |
||
| {{mpl|2013 |
| {{mpl|2013 RH|74}} || align=center | 2013 || CSS || {{MPC|2013+RH74}} |
||
|- |
|- |
||
| {{mpl|2011 MD}} || align=center | 2011 || [[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{MPC|2011+MD}}<sup>(B)</sup> |
| {{mpl|2011 MD}} || align=center | 2011 || [[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{MPC|2011+MD}}<sup>(B)</sup> |
||
Line 74: | Line 68: | ||
| {{mpl|2005 HC|4}} || align=center | 2005 || [[LONEOS]] || {{MPC|2005+HC4}} |
| {{mpl|2005 HC|4}} || align=center | 2005 || [[LONEOS]] || {{MPC|2005+HC4}} |
||
|- |
|- |
||
| {{mpl|2004 XP|14}} || align=center | 2004 || LINEAR || {{MPC|2004+XP14}} |
| {{mpl|(612901) 2004 XP|14}} || align=center | 2004 || LINEAR || {{MPC|2004+XP14}} |
||
|- |
|- |
||
| {{mpl|(374158) 2004 UL}} || align=center | 2004 || LINEAR || {{LoMP|374158|List}} |
| {{mpl|(374158) 2004 UL}} || align=center | 2004 || LINEAR || {{LoMP|374158|List}} |
||
Line 92: | Line 86: | ||
| [[54509 YORP]] || align=center | 2000 || [[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{LoMP|54509|List}} |
| [[54509 YORP]] || align=center | 2000 || [[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{LoMP|54509|List}} |
||
|- |
|- |
||
| [[162173 Ryugu]] || align=center | 1999 ||[[Lincoln Near-Earth Asteroid Research|LINEAR]] || |
| [[162173 Ryugu]] || align=center | 1999 ||[[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{LoMP|162173|List}} |
||
|- |
|- |
||
| {{mpl|(137108) 1999 AN|10}} || align=center | 1999 || [[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{LoMP|137108|List}} |
| {{mpl|(137108) 1999 AN|10}} || align=center | 1999 || [[Lincoln Near-Earth Asteroid Research|LINEAR]] || {{LoMP|137108|List}} |
||
Line 138: | Line 132: | ||
| [[4015 Wilson–Harrington]] || align=center | 1979 || [[Eleanor F. Helin]] || {{LoMP|4015|List}} |
| [[4015 Wilson–Harrington]] || align=center | 1979 || [[Eleanor F. Helin]] || {{LoMP|4015|List}} |
||
|- |
|- |
||
| [[3200 Phaethon]] || align=center | 1983 || [[Simon F. Green]], [[John K.Davies]] / [[IRAS]] || {{LoMP|3200|List}} |
| [[3200 Phaethon]] || align=center | 1983 || [[Simon F. Green]], [[John K. Davies (astronomer)|John K.Davies]] / [[IRAS]] || {{LoMP|3200|List}} |
||
|- |
|- |
||
| [[2063 Bacchus]] || align=center | 1977 || [[Charles T. Kowal]] || {{LoMP|2063|List}} |
| [[2063 Bacchus]] || align=center | 1977 || [[Charles T. Kowal]] || {{LoMP|2063|List}} |
||
Line 172: | Line 166: | ||
* [[Aten asteroid]] |
* [[Aten asteroid]] |
||
* [[List of minor planets]] |
* [[List of minor planets]] |
||
*[[2020 PP1]] |
|||
== References == |
== References == |
||
Line 180: | Line 175: | ||
|publisher = JPL – NASA |
|publisher = JPL – NASA |
||
|url = http://neo.jpl.nasa.gov/neo/groups.html |
|url = http://neo.jpl.nasa.gov/neo/groups.html |
||
|archive-url = https://web.archive.org/web/20020202160655/http://neo.jpl.nasa.gov/neo/groups.html |
|||
|url-status = dead |
|||
|archive-date = 2 February 2002 |
|||
|access-date= 11 November 2016}}</ref> |
|access-date= 11 November 2016}}</ref> |
||
Line 187: | Line 185: | ||
|publisher = Wolfram Research |
|publisher = Wolfram Research |
||
|url = http://scienceworld.wolfram.com/astronomy/ApolloAsteroid.html |
|url = http://scienceworld.wolfram.com/astronomy/ApolloAsteroid.html |
||
| |
|access-date = 27 February 2013}}</ref> |
||
<ref name="neo-jpl-stats">{{cite web |
<ref name="neo-jpl-stats">{{cite web |
||
|title = NEO Discovery Statistics |
|title = NEO Discovery Statistics |
||
|url = http://neo.jpl.nasa.gov/stats/ |
|url = http://neo.jpl.nasa.gov/stats/ |
||
|archive-url = https://web.archive.org/web/20040513230213/http://neo.jpl.nasa.gov/stats/ |
|||
⚫ | |||
|url-status = dead |
|||
|archive-date = 13 May 2004 |
|||
⚫ | |||
<!-- not used |
<!-- not used |
||
Line 199: | Line 199: | ||
|title = numbered objects and orbital class (APO) |
|title = numbered objects and orbital class (APO) |
||
|publisher = [[JPL Solar System Dynamics]] |
|publisher = [[JPL Solar System Dynamics]] |
||
|url = http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=all;obj_numbered=num;ast_orbit_class=APO;OBJ_field=0;ORB_field=0;table_format=HTML;max_rows=50;format_option=comp;c_fields=AcBhBgBjBiBnBsAi;.cgifields=format_option;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=ast_orbit_class;.cgifields=table_format;.cgifields=com_orbit_class&query=1&c_sort=AcA | |
|url = http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=all;obj_numbered=num;ast_orbit_class=APO;OBJ_field=0;ORB_field=0;table_format=HTML;max_rows=50;format_option=comp;c_fields=AcBhBgBjBiBnBsAi;.cgifields=format_option;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=ast_orbit_class;.cgifields=table_format;.cgifields=com_orbit_class&query=1&c_sort=AcA |access-date = 11 November 2016}}</ref>--> |
||
<ref name="pha-apollo">{{cite web |
<!-- unused <ref name="pha-apollo">{{cite web |
||
|title = JPL Small-Body Database Search Engine: PHAs and orbital class (APO) |
|title = JPL Small-Body Database Search Engine: PHAs and orbital class (APO) |
||
|publisher = JPL Solar System Dynamics |
|publisher = JPL Solar System Dynamics |
||
|url = http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=pha;obj_kind=all;obj_numbered=all;ast_orbit_class=APO;OBJ_field=0;ORB_field=0;table_format=HTML;max_rows=100;format_option=comp;c_fields=AcBhBgBjBiBnBsCjCpAi;.cgifields=format_option;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=ast_orbit_class;.cgifields=table_format;.cgifields=com_orbit_class&query=1&c_sort=AcA | |
|url = http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=pha;obj_kind=all;obj_numbered=all;ast_orbit_class=APO;OBJ_field=0;ORB_field=0;table_format=HTML;max_rows=100;format_option=comp;c_fields=AcBhBgBjBiBnBsCjCpAi;.cgifields=format_option;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=ast_orbit_class;.cgifields=table_format;.cgifields=com_orbit_class&query=1&c_sort=AcA |access-date = 11 November 2016}}</ref> --> |
||
<ref name="USA-Today-Chelyabinsk">{{cite web |
<ref name="USA-Today-Chelyabinsk">{{cite web |
||
Line 212: | Line 212: | ||
|date = 26 February 2013 |
|date = 26 February 2013 |
||
|url = https://www.usatoday.com/story/tech/2013/02/26/meteor-russia-apollo-space/1948673/ |
|url = https://www.usatoday.com/story/tech/2013/02/26/meteor-russia-apollo-space/1948673/ |
||
| |
|access-date = 11 November 2016}}</ref> |
||
<ref name="NewScientist-Chelyabinsk">{{cite web |
<ref name="NewScientist-Chelyabinsk">{{cite web |
||
Line 220: | Line 220: | ||
|date = 26 February 2013 |
|date = 26 February 2013 |
||
|url = https://www.newscientist.com/article/dn23213-russian-meteor-traced-to-apollo-asteroid-family/ |
|url = https://www.newscientist.com/article/dn23213-russian-meteor-traced-to-apollo-asteroid-family/ |
||
| |
|access-date = 11 November 2016}}</ref> |
||
}} <!-- end of reflist --> |
}} <!-- end of reflist --> |
Latest revision as of 08:41, 30 October 2024
The Apollo asteroids are a group of near-Earth asteroids named after 1862 Apollo, discovered by German astronomer Karl Reinmuth in the 1930s. They are Earth-crossing asteroids that have an orbital semi-major axis greater than that of the Earth (a > 1 AU) but perihelion distances less than the Earth's aphelion distance (q < 1.017 AU).[1][2]
As of October 2024[update], the number of known Apollo asteroids is 20,412, making the class the largest group of near-Earth objects (cf. the Aten, Amor and Atira asteroids),[3] of which 1,628 are numbered (asteroids are not numbered until they have been observed at two or more oppositions), 79 are named, and 2,104 are identified as potentially hazardous asteroids.[4][5]
The closer their semi-major axis is to Earth's, the less eccentricity is needed for the orbits to cross. The Chelyabinsk meteor, that exploded over the city of Chelyabinsk in the southern Urals region of Russia on February 15, 2013, injuring an estimated 1,500 people with flying glass from broken windows, was an Apollo-class asteroid.[6][7]
List
[edit]The largest known Apollo asteroid is 1866 Sisyphus, with a diameter of about 8.5 km. Examples of known Apollo asteroids include:
See also
[edit]- Alinda group
- Amor asteroid
- Apollo asteroids (category)
- Apollo asteroid records
- Aten asteroid
- List of minor planets
- 2020 PP1
References
[edit]- ^ "Near-Earth Object Groups". JPL – NASA. Archived from the original on 2 February 2002. Retrieved 11 November 2016.
- ^ Weisstein, Eric. "Apollo Asteroid". Wolfram Research. Retrieved 27 February 2013.
- ^ "NEO Discovery Statistics". Archived from the original on 13 May 2004. Retrieved 11 November 2016.
- ^ "Small-Body Database Query". Solar System Dynamics – Jet Propulsion Laboratory. NASA – California Institute of Technology. Retrieved 2024-10-11.
- ^ "List of Apollo Minor Planets". IAU Minor Planet Center. Center for Astrophysics. Retrieved 2024-10-11.
- ^ Cantor, Matt (26 February 2013). "Scientists figure out Russia meteor's origin". USA Today. Retrieved 11 November 2016.
- ^ Jacob Aron (26 February 2013). "Russian meteor traced to Apollo asteroid family". New Scientist. Retrieved 11 November 2016.
- ^ The Spacewatch Project, Arizona Board of Regents, 2010