2017 BQ6

{{short description|Asteroid}}

{{DISPLAYTITLE:{{mp|2017 BQ|6}}}}

{{use dmy dates|date=February 2018}}

{{Infobox planet

| minorplanet = yes

| name = {{mp|2017 BQ|6}}

| background = #FFC2E0

| image = 2017 BQ6 radar rotation.gif

| image_scale =

| caption = Radar image of {{mp|2017 BQ|6}}

| discovery_ref =

| discoverer = Space Surveillance Telescope

| discovered = Lincoln Lab's ETS

| mpc_name = {{mp|2017 BQ|6}}

| alt_names = E2017-C83

| pronounced =

| named_after =

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

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 3

| observation_arc = 130 days

| aphelion = 2.9802 AU

| perihelion = 0.9133 AU

| semimajor = 1.9468 AU

| eccentricity = 0.5309

| period = 2.72 yr (992 days)

| mean_anomaly = 65.132°

| mean_motion = {{Deg2DMS|0.3628|sup=ms}} / day

| inclination = 9.0020°

| asc_node = 133.03°

| arg_peri = 43.562°

| moid = 0.0132 AU (5.1 LD)

| dimensions = {{val|0.120|0.027|u=km}}

| rotation = {{val|2.150}} h
3 h

| albedo = {{val|0.13|0.103|0.057}}

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

| abs_magnitude = 21.4

}}

{{mp|2017 BQ|6}} is a sub-kilometer asteroid on an eccentric orbit, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 150 meters in diameter. It was discovered on 26 January 2017, by the Space Surveillance Telescope at Lincoln Laboratory's ETS (Atom Site) and passed within 6.6 lunar distances of Earth on 7 February 2017 at 6:36 UT.

Radar imaging

Its closest approach was observed by NASA's Goldstone Solar System Radar in California's Mojave Desert, determining it to have a number of angular flat surfaces similar to a polyhedral die.

File:PIA21452 - Angular Asteroid Composite.jpg

{{clear|left}}

Orbit

{{mp|2017 BQ|6}} orbits the Sun with a semi-major axis of 1.95 AU at a distance of 0.9–3.0 AU once every 2 years and 9 months (992 days). Its orbit has an eccentricity of 0.53 and an inclination of 9° with respect to the ecliptic. It has an Earth minimum orbital intersection distance of {{convert |0.0132 |AU |km |abbr=on |lk=off |sigfig= 3}}, which corresponds to 5.1 lunar distances.

File:2017BQ6.png

{{clear|left}}

Physical characteristics

Based on an absolute magnitude of 21.4 and an assumed albedo for stony S-type asteroids of 0.20, {{mp|2017 BQ|6}} measures 156 meters in diameter. The body has a rotation period of 2.15 hours and a brightness amplitude of 0.38 magnitude ({{small|U=2}}).

References

{{reflist|30em|refs=

{{cite web

|type = 2017-06-05 last obs.

|title = JPL Small-Body Database Browser: (2017 BQ6)

|url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3767007

|publisher = Jet Propulsion Laboratory

|accessdate = 21 November 2017}}

{{cite web

|title = 2017 BQ6

|work = Minor Planet Center

|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=2017+BQ6

|accessdate = 21 November 2017}}

{{cite web

|title = LCDB Data for 2017 BQ6

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=0%7C2017+BQ6

|accessdate = 21 November 2017}}

{{cite journal

|title = Physical Properties of 299 NEOs Manually Recovered in Over Five Years of NEOWISE Survey Data

|first1 = Joseph |last1 = Masiero

|first2 = Patrice |last2 = Smith

|first3 = Lean D. |last3 = Teodoro

|first4 = A. K. |last4 = Mainzer

|first5 = R. M. |last5 = Cutri

|first6 = T. |last6 = Grav

|first7 = E. L. |last7 = Wright

|journal = The Planetary Science Journal |arxiv = 2003.14406

|date = 1 April 2020|volume = 1 |issue = 1 |page = 9 |doi = 10.3847/PSJ/ab8638 |bibcode = 2020PSJ.....1....9M |s2cid = 214727881 |doi-access = free }}

}}