(6178) 1986 DA

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Asteroid

title: "(6178) 1986 DA" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["amor-asteroids", "radar-imaged-asteroids", "discoveries-by-minoru-kizawa", "astronomical-objects-discovered-in-1986"] description: "Asteroid" topic_path: "general/amor-asteroids" source: "https://en.wikipedia.org/wiki/(6178)_1986_DA" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

::summary Asteroid ::

::data[format=table title="Infobox planet"]

Field	Value
minorplanet	yes
name	(6178) 1986 DA
background	#FFC2E0
discovery_ref
discovered	16 February 1986
discoverer	M. Kizawa
discovery_site	Shizuoka Obs.
mpc_name	(6178) 1986 DA
alt_names	1986 DA
mp_category	Amor NEO
orbit_ref
epoch	4 September 2017 (JD 2458000.5)
uncertainty	0
observation_arc	38.03 yr (13,890 days)
aphelion	4.4648 AU
perihelion	1.1805 AU
semimajor	2.8226 AU
eccentricity	0.5818
period	4.74 yr (1,732 days)
mean_anomaly	233.20°
mean_motion	/ day
inclination	4.3056°
asc_node	64.643°
arg_peri	127.36°
moid	0.1922 AU 74.9 LD
jupiter_moid	0.5212 AU
mean_diameter	2.3 km (dated)
km
3.15 km (taken)
km
rotation	3.50 h
h
albedo
0.15

| spectral_type = M B–V = 0.677 U–B = 0.267 | abs_magnitude = 15.1 (R)16.11

**** is a metallic asteroid, classified as near-Earth object of the Amor group, approximately 3 kilometers in diameter. It was discovered on 16 February 1986, by Japanese astronomer Minoru Kizawa at Shizuoka Observatory, Japan.

1986 DA was the first near Earth asteroid thought to be of metallic composition, with high radar brightness; with that it was predicted to have 100 thousand tons of platinum group metals including gold and suggested as a resource for future space colonists.

Orbit and classification

As an eccentric Amor asteroid has an Earth minimum orbit intersection distance of 0.1922 AU and approaches the orbit of Earth from the outside but does not cross it. It crosses however the orbit of Mars and can be classified as a Mars-crosser and also approaches the orbit of Jupiter within 0.5 AU. The asteroid orbits the Sun at a distance of 1.2–4.5 AU once every 4 years and 9 months (1,732 days). Its orbit has an eccentricity of 0.58 and an inclination of 4° with respect to the ecliptic. The first precovery was taken at Siding Spring Observatory in 1977, extending the asteroid's observation arc by 9 years prior to its discovery.

Physical characteristics

The metallic M-type asteroid is notable for being significantly more radar-reflective than other asteroids. Radar measurements suggest it is composed of nickel and iron and that it was derived from the center of a much larger object that experienced melting and differentiation. The observed radar albedo was 0.58 and the optical albedo was 0.14.

Rotation and shape

It was most probably formed from a larger body through a catastrophic collision with another object. Radar measurements of this body indicate that the surface is relatively smooth on scales of less than a meter, but it is highly irregular on scales of 10–100 meters. Several lightcurve analysis gave it a concurring rotation period of 3.50 to 3.51 hours with a relatively high brightness amplitude between 0.03 and 0.48 in magnitude, indicating an irregular shape ().

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid has an albedo of 0.08 and 0.16, and a diameter of 3.1 to 3.2 kilometers, respectively. The Collaborative Asteroid Lightcurve Link selects 3.15 kilometers as best result, while the first estimate from 1994 gave a diameter of 2.3 kilometers.

Mining considerations

The asteroid achieved its most notable recognition when scientists revealed that it contained over "10,000 tons of gold and 100,000 tons of platinum", or an approximate value at the time of its discovery of "$90 billion for the gold and a cool trillion dollars for the platinum, plus loose change for the asteroid's 10 billion tons of iron and a billion tons of nickel." In 2024 the estimated value of 100,000 tons of platinum was worth approximately 3.4 trillion US dollars. The delta-v for a spacecraft rendezvous with this asteroid from low Earth orbit is 7.1 km/s.

Notes

References

|type = 2015-07-28 last obs. |title = JPL Small-Body Database Browser: 6178 (1986 DA) |url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2006178 |publisher = Jet Propulsion Laboratory |accessdate = 26 May 2017}}

|title = 6178 (1986 DA) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=6178 |accessdate = 26 May 2016}}

|title = Delta-v for spacecraft rendezvous with all known near-Earth asteroids |publisher = NASA |date = 2006-06-01 |url = http://echo.jpl.nasa.gov/~lance/delta_v/delta_v.rendezvous.html |archive-url = https://web.archive.org/web/20010603042837/http://echo.jpl.nasa.gov/~lance/delta_v/delta_v.rendezvous.html |url-status = dead |archive-date = 2001-06-03 |accessdate = 8 June 2006}}

|title = LCDB Data for (6178) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=6178%7C |accessdate = 26 May 2016}}

|first1 = Petr |last1 = Pravec |first2 = Alan W. |last2 = Harris |first3 = Peter |last3 = Kusnirák |first4 = Adrián |last4 = Galád |first5 = Kamil |last5 = Hornoch |date = September 2012 |title = Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations |journal = Icarus |volume = 221 |issue = 1 |pages = 365–387 |bibcode = 2012Icar..221..365P |doi = 10.1016/j.icarus.2012.07.026}}

|display-authors = 6 |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |first7 = R. S. |last7 = McMillan |first8 = T. |last8 = Spahr |first9 = R. M. |last9 = Cutri |first10 = E. |last10 = Wright |first11 = J. |last11 = Watkins |first12 = W. |last12 = Mo |first13 = C. |last13 = Maleszewski |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407|s2cid = 118700974 }}

|author = Wisniewski, W. Z. |date = June 1987 |title = Photometry of six radar target asteroids |journal = Icarus |pages = 566–572 |issn = 0019-1035 |bibcode = 1987Icar...70..566W |doi = 10.1016/0019-1035(87)90096-0 |volume =70 |issue = 3}}

|author = Zeigler, K. W. |date = March 1990 |title = Photoelectric Photometry of Asteroids 81 Terpsichore, 381 Myrrha, and 1986 DA |journal = The Minor Planet Bulletin |volume = 17 |page = 1 |bibcode = 1990MPBu...17....1Z}}

References

"Near-Earth Metal Asteroid Discovered".

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