1704 Wachmann

{{Short description|Main-belt asteroid}}

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

{{Infobox planet

| minorplanet = yes

| name = 1704 Wachmann

| background = #D6D6D6

| image = 1704Wachmann (Lightcurve Inversion).png

| image_scale =

| caption = {{longitem|Light curve based 3D-model of Wachmann|style=padding: 5px 0;}}

| discovery_ref =

| discovered = 7 March 1924

| discoverer = K. Reinmuth

| discovery_site = Heidelberg Obs.

| mpc_name = (1704) Wachmann

| alt_names = A924 EE{{·}}1947 CE
1957 BJ

| pronounced =

| named_after = Arno Wachmann
{{small|(German astronomer)}}

| mp_category = main-belt{{·}}{{small|(inner)}}

| orbit_ref =

| epoch = 4 September 2017 (JD 2458000.5)

| uncertainty = 0

| observation_arc = 93.16 yr (34,026 days)

| aphelion = 2.4163 AU

| perihelion = 2.0292 AU

| semimajor = 2.2228 AU

| eccentricity = 0.0871

| period = 3.31 yr (1,210 days)

| mean_anomaly = 67.047°

| mean_motion = {{Deg2DMS|0.2974|sup=ms}} / day

| inclination = 0.9715°

| asc_node = 259.47°

| arg_peri = 280.77°

| dimensions = {{val|6.618|0.070}}
{{val|6.934|0.070}} km
7.82 km {{small|(calculated)}}

| rotation = {{val|3.314|0.001}} h

| albedo = {{val|0.1767|0.0133}}
{{val|0.193|0.036}}
0.20 {{small|(assumed)}}

| spectral_type = S

| abs_magnitude = 12.9{{·}}{{val|12.97|0.13}}{{·}}13.3

}}

1704 Wachmann, provisional designation {{mp|A924 EE}}, is a stony asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by German astronomer Karl Reinmuth at Heidelberg Observatory on 7 March 1924. It was later named after astronomer Arno Wachmann.

Classification and orbit

The S-type asteroid orbits the Sun in the inner main-belt at a distance of 2.0–2.4 AU once every 3 years and 4 months (1,210 days). Its orbit has an eccentricity of 0.09 and an inclination of 1° with respect to the ecliptic. No precoveries were taken. The asteroid's observation arc begins 3 days after its official discovery observation.

Physical characteristics

= Lightcurves =

In April 2007, a rotational lightcurve Wachmann was obtained at the U.S. Sandia View Observatory in New Mexico ({{small|H03}}). Lightcurve analysis gave a well-defined rotation period of {{val|3.314|0.001}} hours with a brightness variation of 0.40 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, Wachmann measures 6.6 and 6.9 kilometers in diameter, and its surface has an albedo of 0.177 and 0.193, respectively, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 7.8 kilometers, based on an absolute magnitude of 12.9.

Naming

This minor planet was named for Arno Wachmann (1902–1990), long-time astronomer at the Bergedorf Observatory in Hamburg, discoverer of minor planets and comets, and observer of variable and binary stars. He is best known for the co-discovery of the three "Schwassmann–Wachmann" comets, 29P, 31P and 73P. The official {{MoMP|1704|naming citation}} was published by the Minor Planet Center on 20 February 1976 ({{small|M.P.C. 3933}}).

References

{{reflist|refs=

{{cite web

|type = 2017-05-05 last obs.

|title = JPL Small-Body Database Browser: 1704 Wachmann (A924 EE)

|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001704

|publisher = Jet Propulsion Laboratory

|accessdate = 7 June 2017}}

{{cite book

|title = Dictionary of Minor Planet Names – (1704) Wachmann

|last = Schmadel | first = Lutz D.

|publisher = Springer Berlin Heidelberg

|pages = 135–136

|date = 2007

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

|doi = 10.1007/978-3-540-29925-7_1705 |chapter = (1704) Wachmann }}

{{cite web

|title = 1704 Wachmann (A924 EE)

|work = Minor Planet Center

|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=1704

|accessdate = 20 July 2016}}

{{cite book

|title = Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)

|chapter = Appendix – Publication Dates of the MPCs

|last = Schmadel |first=Lutz D.

|publisher = Springer Berlin Heidelberg

|page = 221

|isbn = 978-3-642-01964-7

|doi = 10.1007/978-3-642-01965-4}}

{{cite web

|title = LCDB Data for (1704) Wachmann

|publisher = Asteroid Lightcurve Database (LCDB)

|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1704%7CWachmann

|accessdate = 20 July 2016}}

{{cite journal

|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}}

{{Cite journal

|last = Julian, II

|first = William M.

|date = March 2008

|title = Period Determination for 1704 Wachmann

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35....4J

|journal = The Minor Planet Bulletin

|volume = 35

|issue = 1

|page = 4

|issn = 1052-8091

|bibcode = 2008MPBu...35....4J

|access-date= 20 July 2016}}

{{cite journal

|display-authors = 6

|first1 = Peter |last1 = Veres

|first2 = Robert |last2 = Jedicke

|first3 = Alan |last3 = Fitzsimmons

|first4 = Larry |last4 = Denneau

|first5 = Mikael |last5 = Granvik

|first6 = Bryce |last6 = Bolin

|first7 = Serge |last7 = Chastel

|first8 = Richard J. |last8 = Wainscoat

|first9 = William S. |last9 = Burgett

|first10 = Kenneth C. |last10 = Chambers

|first11 = Heather |last11 = Flewelling

|first12 = Nick |last12 = Kaiser

|first13 = Eugen A. |last13 = Magnier

|first14 = Jeff S. |last14 = Morgan

|first15 = Paul A. |last15 = Price

|first16 = John L. |last16 = Tonry

|first17 = Christopher |last17 = Waters

|date = November 2015

|title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V

|journal = Icarus

|volume = 261

|pages = 34–47

|bibcode = 2015Icar..261...34V

|doi = 10.1016/j.icarus.2015.08.007

|arxiv = 1506.00762

|access-date= 20 July 2016}}

{{cite journal

|display-authors = 6

|first1 = Joseph R. |last1 = Masiero

|first2 = T. |last2 = Grav

|first3 = A. K. |last3 = Mainzer

|first4 = C. R. |last4 = Nugent

|first5 = J. M. |last5 = Bauer

|first6 = R. |last6 = Stevenson

|first7 = S. |last7 = Sonnett

|date = August 2014

|title = Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos

|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M

|journal = The Astrophysical Journal

|volume = 791

|issue = 2

|page = 11

|bibcode = 2014ApJ...791..121M

|doi = 10.1088/0004-637X/791/2/121

|arxiv = 1406.6645

|access-date= 8 December 2016}}

}}