(159857) 2004 LJ1

{{Short description|Asteroid on an eccentric orbit}}

{{DISPLAYTITLE:{{mp|(159857) 2004 LJ|1}}}}

{{Use dmy dates|date=September 2020}}

{{Infobox planet

| minorplanet = yes

| name = {{mp|(159857) 2004 LJ|1}}

| background = #FFC2E0

| image =

| image_size =

| caption =

| discovery_ref =

| discoverer = LINEAR

| discovery_site = Lincoln Lab's ETS

| discovered = 10 June 2004

| mpc_name = {{mp|(159857) 2004 LJ|1}}

| alt_names = {{mp|2004 LJ|1}}

| pronounced =

| named_after =

| mp_category = {{nowrap|Apollo{{·}}NEO{{·}}PHA}}

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 0

| observation_arc = 22.29 yr (8,141 days)

| aphelion = 3.6072 AU

| perihelion = 0.9203 AU

| semimajor = 2.2637 AU

| eccentricity = 0.5935

| period = 3.41 yr (1,244 days)

| mean_anomaly = 286.61°

| mean_motion = {{Deg2DMS|0.2894|sup=ms}} / day

| inclination = 23.140°

| asc_node = 235.58°

| arg_peri = 139.97°

| moid = 0.0168 AU{{·}}6.5 LD

| mean_diameter = 2.47 km {{small|(calculated)}}
{{val|3.070|1.324}} km

| rotation = {{val|2.661|0.001}} h{{efn|name=lightcurve-plots-Warner}}
{{val|2.7247|0.0002}} h
{{val|2.76}} h{{efn|name=lcdb-Torppa-2011}}

| albedo = {{val|0.130|0.158}}
0.20 {{small|(assumed)}}

| spectral_type = S {{small|(assumed)}}

| abs_magnitude = {{val|15.11|0.94}}{{·}}15.4

}}

{{mp|(159857) 2004 LJ|1}}, provisional designation {{mp|2004 LJ|1}}, is an asteroid on an eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 3 kilometers in diameter. The asteroid was discovered on 10 June 2004, by astronomers of the LINEAR program at Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. It is one of the largest potentially hazardous asteroids known to exist.

Orbit and classification

{{mp|2004 LJ|1}} is a member of the dynamical Apollo group, which are Earth-crossing asteroids. Apollo asteroids are the largest subgroup of near-Earth objects.

The body orbits the Sun at a distance of 0.9–3.6 AU once every 3 years and 5 months (1,244 days; semi-major axis of 2.26 AU). Its orbit has an eccentricity of 0.59 and an inclination of 23° with respect to the ecliptic. Its observation arc begins with a precovery from the Digitized Sky Survey taken at the Siding Spring Observatory, Australia, in February 1995, more than 9 years prior to its official discovery observation at Socorro.

= Close approaches =

With an absolute magnitude of at least 15.4, {{mp|2004 LJ|1}} is one of the brightest and presumably largest known potentially hazardous asteroid (see PHA-list). It has an Earth minimum orbital intersection distance of {{convert |0.0168 |AU |km |abbr=on |lk=off |sigfig=3}}, which translates into 6.5 lunar distances (LD). On 16 November 2038, this asteroid will make its closest near-Earth encounter at a nominal distance of 0.0198 AU (7.7 LD). It is also classified as a Mars-crosser, crossing the orbit of the Red Planet at 1.66 AU.

{{Large near earth asteroid flybys 10LD}}

Physical characteristics

{{mp|2004 LJ|1}} is an assumed stony S-type asteroid.

= Rotation period =

Three rotational lightcurves of {{mp|2004 LJ|1}} have been obtained from photometric observations by Johanna Torppa, Adrián Galád and Brian Warner since 2004.{{efn|name=lightcurve-plots-Warner}}{{efn|name=lcdb-Torppa-2011}} Lightcurve analysis gave a consolidated rotation period of 2.7247 hours with a brightness amplitude between 0.15 and 0.59 magnitude ({{small|U=3}}).

= Diameter and albedo =

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, {{mp|2004 LJ|1}} measures 3.07 kilometers in diameter and its surface has an albedo of 0.13. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 2.47 kilometers, based on an absolute magnitude of 15.4.

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 30 June 2007. As of 2018, it has not been named.

Notes

{{notelist|refs=

{{efn|name=lcdb-Torppa-2011|1=Torppa (2011) web: Undated observation. Rotation period {{val|2.76}} hours with a brightness amplitude of {{val|0.5}} mag. Quality Code of 2. Summary figures at the [http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=159857%7C LCDB]}}

{{efn|name=lightcurve-plots-Warner|1=[http://www.planetarysciences.org/plots/BDW/159857_2004LJ1_2014-06-25.PNG Lightcurve plot of {{mp|(159857) 2004 LJ|1}}] from June to July 2014, by B. D. Warner at the CS3–Palmer Divide Station in California ({{small|U82}}). Quality code of 2. Summary figures at the [http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=159857%7C LCDB] and [http://www.planetarysciences.org CS3 website].}}

}}

References

{{reflist|30em|refs=

{{cite web

|type = 2017-05-19 last obs.

|title = JPL Small-Body Database Browser: 159857 (2004 LJ1)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2159857

|publisher = Jet Propulsion Laboratory

|accessdate = 18 January 2018}}

{{cite web

|title = 159857 (2004 LJ1)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=159857

|accessdate = 18 January 2018}}

{{cite web

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|work = Minor Planet Center

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|accessdate = 24 February 2018}}

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|work = Minor Planet Center

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|accessdate = 18 January 2018}}

{{cite web

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|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=159857%7C

|accessdate = 18 January 2018}}

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{{Cite journal

|author = Warner, Brian D.

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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015MPBu...42...41W

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|access-date= 18 January 2018}}

{{cite journal

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}}