6141 Durda

{{Use dmy dates|date=October 2019}}

{{Infobox planet

| minorplanet = yes

| name = 6141 Durda

| background = #FA8072

| image =

| image_size =

| caption =

| discovery_ref =

| discovered = 26 December 1992

| discoverer = Spacewatch

| discovery_site = Kitt Peak National Obs.

| mpc_name = (6141) Durda

| alt_names = {{mp|1992 YC|3}}{{·}}{{mp|1983 AZ|2}}
1988 AJ{{·}}1989 PL

| pronounced =

| named_after = Daniel D. Durda
{{small|(astronomer, artist)}}

| mp_category = Mars-crosser{{·}}Hungaria

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 0

| observation_arc = 34.05 yr (12,435 days)

| aphelion = 2.0780 AU

| perihelion = 1.5580 AU

| semimajor = 1.8180 AU

| eccentricity = 0.1430

| period = 2.45 yr (895 days)

| mean_anomaly = 55.898°

| mean_motion = {{Deg2DMS|0.4021|sup=ms}} / day

| inclination = 16.454°

| asc_node = 284.81°

| arg_peri = 145.73°

| dimensions = 3.20 km {{small|(calculated)}}
4 km {{small|(est. at 0.25)}}

| rotation = {{val|460|5}} h

| albedo = 0.30 {{small|(assumed)}}

| spectral_type = E

| abs_magnitude = 14.4

}}

6141 Durda, provisional designation {{mp|1992 YC3}} is a stony Hungaria asteroid, classified as slow rotator and Mars-crosser from the innermost region of the asteroid belt, approximately 3.2 kilometers in diameter. It was discovered on 26 December 1992, by Spacewatch at Kitt Peak National Observatory in Arizona, United States.

Classification and orbit

This Mars-crosser and presumed E-type asteroid is also member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun in the inner main-belt at a distance of 1.6–2.1 AU once every 2 years and 5 months (895 days). Its orbit has an eccentricity of 0.14 and an inclination of 16° with respect to the ecliptic. On 22 September 2154, it will pass {{convert|0.0088|AU|km|abbr=on|lk=off}} from Mars. Durda was first identified as {{mp|1983 AZ|2}} at Karl Schwarzschild Observatory in 1983, extending the body's observation arc by 9 years prior to its official discovery observation at Kitt Peak.

Lightcurve

In October 2009, a rotational lightcurve was obtained from photometric observations by Brian Warner at the Palmer Divide Station in Colorado. Lightcurve analysis gave a rotation period of {{val|460|5}} hours with a brightness variation of 0.50 magnitude ({{small|U=2+}}). Durda belongs to the Top 100 slow rotators known to exists.

Diameter

Based on a magnitude-to-diameter conversion, Durda{{'}}s generic diameter is between 3 and 7 kilometer for an absolute magnitude of 14.4, and an assumed albedo in the range of 0.05 to 0.25. Since asteroids in the inner main-belt are typically of stony rather than carbonaceous composition, with albedos above 0.20, Durda{{'}}s diameter can be estimate to measure around 4 kilometers, as the higher its albedo (reflectivity), the lower the body's diameter. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.30 – a compromise value between 0.4 and 0.2, corresponding to the Hungaria asteroids both as family and orbital group – and calculates a diameter of 3.20 kilometers.

Naming

This minor planet was named in honor of American planetary scientist Daniel D. Durda, who has researched the generation, evolution, size distribution and fragmentation of minor planets, resulting in the formation of minor-planet moons. He was especially interested in (243) Ida I Dactyl when he was member of the Galileo mission team. Daniel Durda is also a pilot and an artist of astronomical paintings. In 2015, he was awarded the Carl Sagan Medal for "communicating the wonder of planetary science through visual artistry". The approved naming citation was published by the Minor Planet Center on 8 August 1998 ({{small|M.P.C. 32345}}).

References

{{reflist|30em|refs=

{{cite web

|type = 2017-01-23 last obs.

|title = JPL Small-Body Database Browser: 6141 Durda (1992 YC3)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2006141

|publisher = Jet Propulsion Laboratory

|access-date = 4 July 2017}}

{{cite book

|title = Dictionary of Minor Planet Names – (6141) Durda

|last = Schmadel | first = Lutz D.

|publisher = Springer Berlin Heidelberg

|page = 512

|date = 2007

|isbn = 978-3-540-00238-3

|doi = 10.1007/978-3-540-29925-7_5671 |chapter = (6141) Durda }}

{{cite web

|title = 6141 Durda (1992 YC3)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=6141

|access-date = 12 March 2017}}

{{cite web

|title = MPC/MPO/MPS Archive

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html

|access-date = 12 March 2017}}

{{cite web

|title = 2015 Prize Recipients: Dan Durda - 2015 Carl Sagan Medal

|publisher = AAS – American Astronomical Society, Division for Planetary Sciences

|url = https://dps.aas.org/prizes/2015

|access-date = 12 March 2017}}

{{cite web

|title = LCDB Data for (6141) Durda

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=6141%7CDurda

|access-date = 12 March 2017}}

{{Cite journal

|author = Warner, Brian D.

|date = April 2010

|title = Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 September-December

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37...57W

|journal = The Minor Planet Bulletin

|volume = 37

|issue = 2

|pages = 57–64

|issn = 1052-8091

|bibcode = 2010MPBu...37...57W

|access-date= 12 March 2017}}

{{cite web

|title = Absolute Magnitude (H)

|publisher = NASA/JPL – Near Earth Object Program

|url = http://neo.jpl.nasa.gov/glossary/h.html

|archive-url = https://web.archive.org/web/20010302182040/http://neo.jpl.nasa.gov/glossary/h.html

|url-status = dead

|archive-date = 2 March 2001

|access-date = 12 March 2017}}

}}