9564 Jeffwynn

Last updated

9564 Jeffwynn
Discovery [1]
Discovered by C. S. Shoemaker
E. M. Shoemaker
Discovery site Palomar Obs.
Discovery date26 September 1987
Designations
(9564) Jeffwynn
Named after
Jeffrey Wynn
(American geophysicist) [2]
1987 SG3 ·1951 NQ
Mars-crosser [1] [3]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 65.68 yr (23,988 days)
Aphelion 3.0828 AU
Perihelion 1.5962 AU
2.3395 AU
Eccentricity 0.3177
3.58 yr (1,307 days)
159.61°
0° 16m 31.44s / day
Inclination 22.307°
187.10°
121.61°
Physical characteristics
Dimensions4.71 km (calculated) [3]
3.035±0.001 h [4] [lower-alpha 1]
0.20 (assumed) [3]
S [3] [5]
13.00 [5]  ·14.0 [1] [3]  ·14.52±0.76 [6]

    9564 Jeffwynn, provisional designation 1987 SG3, is an eccentric asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 4.7 kilometers in diameter.

    Contents

    The asteroid was discovered on 26 September 1987, by American astronomer couple Carolyn and Eugene Shoemaker at Palomar Observatory in California, United States. [7] It was named for American geophysicist Jeffrey C. Wynn. [2]

    Orbit and classification

    Jeffwynn is a stony asteroid that orbits the Sun at a distance of 1.6–3.1  AU once every 3 years and 7 months (1,307 days). Its orbit has an eccentricity of 0.32 and an inclination of 22° with respect to the ecliptic. [1]

    The body's observation arc begins 36 years prior to its official discovery observation, with its precovery identification as 1951 NQ at Palomar in July 1951. [7]

    Physical characteristics

    Jeffwynn has been characterized as a common, stony S-type asteroid by photometry from the Sloan Digital Sky Survey. [3] [5]

    Lightcurves

    In September 2012, a rotational lightcurve of Jeffwynn was obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory ( 716 ) in Colorado. Lightcurve analysis gave a well-defined rotation period of 3.035 hours with a brightness variation of 0.16 magnitude ( U=3 ). [4] [lower-alpha 1]

    Diameter and albedo

    The Collaborative Asteroid Lightcurve Link calculates a diameter of 4.7 kilometers with an absolute magnitude of 14.0 and an assumed albedo for stony asteroids of 0.20. [3]

    Naming

    This minor planet was named in honor of American Jeffrey C. Wynn, research geophysicist with the United States Geological Survey, described as a "humorous, curious, inventive, adventurous geophysicist", who examined the Saudi Arabian Wabar craters on several expeditions in 1994 and 1995, together with Eugene Shoemaker, after whom the minor planet 2074 Shoemaker is named. Wynn's research included mapping the seafloor, analyzing terrestrial minerals, and studying aquifers and archaeological sites. He also observed with the comet-discovering Shoemaker-Levy team. [2] The official naming citation was published by the Minor Planet Center on 23 November 1999 ( M.P.C. 36948). [8]

    Notes

    1. 1 2 Warner (2012): lightcurve plot of (9564) Jeffwynn with a rotation period 3.0350±0.001 hours and a brightness amplitude of 0.16 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL)

    Related Research Articles

    3225 Hoag, provisional designation 1982 QQ, is a dynamical Hungaria asteroid from the innermost regions of the asteroid belt, approximately 5.5 kilometers in diameter. It was discovered on 20 August 1982, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California. The stony S/L-type asteroid has a short rotation period of 2.37 hours. It was named for American astronomer Arthur Hoag.

    <span class="mw-page-title-main">9994 Grotius</span> Rafita asteroid

    9994 Grotius, provisional designation 4028 P-L, is a stony Rafita asteroid from the middle regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered during the Palomar–Leiden survey in 1960, and named after Dutch jurist Hugo Grotius.

    (9992) 1997 TG19 is a stony asteroid and eccentric Mars-crosser, approximately 4 kilometers in diameter. It was discovered on 8 October 1997, by Japanese astronomers Tetsuo Kagawa and Takeshi Urata at Gekko Observatory near Shizuoka, Japan.

    6398 Timhunter, provisional designation 1991 CD1, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 5.5 kilometers in diameter. It was discovered on 10 February 1991, by American astronomer couple Carolyn and Eugene Shoemaker, in collaboration with Canadian astronomer David H. Levy at Palomar Observatory in California, United States. It was named for American amateur astronomer Tim Hunter.

    49777 Cappi is a stony background asteroid from the inner regions of the asteroid belt, approximately 2 kilometers in diameter.

    3070 Aitken, provisional designation 1949 GK, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 4 April 1949, by astronomers of the Indiana Asteroid Program at Goethe Link Observatory in Indiana, United States. The asteroid was named after American astronomer Robert Grant Aitken.

    2744 Birgitta, provisional designation 1975 RB, is a stony asteroid and a Mars-crosser on an eccentric orbit from the innermost regions of the asteroid belt, approximately 3 kilometers in diameter. It was discovered at the Kvistaberg Station of the Uppsala Observatory in Sweden on 4 September 1975, by Swedish astronomer Claes-Ingvar Lagerkvist, who named it after his daughter, Anna Birgitta Angelica Lagerkvist. The S-type asteroid has a rotation period of 9.0 hours.

    5642 Bobbywilliams, provisional designation 1990 OK1, is an eccentric, stony asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 4.7 kilometers in diameter.

    1622 Chacornac is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 15 March 1952, by French astronomer Alfred Schmitt at the Royal Observatory of Belgium in Uccle, and named after astronomer Jean Chacornac.

    3936 Elst, provisional designation 2321 T-3, is a stony Vestian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. The asteroid was discovered on 16 October 1977, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Dutch–American astronomer Tom Gehrels at Palomar Observatory in California, United States. It was named after Belgian astronomer Eric W. Elst.

    5474 Gingasen, provisional designation 1988 XE1, is a Vestian asteroid and suspected binary system from the inner regions of the asteroid belt, approximately 6 kilometers in diameter.

    8013 Gordonmoore, provisional designation 1990 KA, is an eccentric, stony asteroid and near-Earth object of the Apollo group, approximately 1–2 kilometers in diameter.

    3640 Gostin, provisional designation 1985 TR3, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 11 October 1985, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California. The S-type asteroid has a rotation period of 3.26 hours. It was named for Australian geologist Victor Gostin.

    3800 Karayusuf, provisional designation 1984 AB, is a Mars-crossing asteroid and suspected binary system from inside the asteroid belt, approximately 2.5 kilometers in diameter. It was discovered on 4 January 1984, by American astronomer Eleanor Helin at the Palomar Observatory in California. The S/L-type asteroid has a short rotation period of 2.2 hours. It was named after Syrian physician Alford Karayusuf, a friend of the discoverer.

    11118 Modra is a Flora asteroid of uncertain composition from the inner regions of the asteroid belt, approximately 5 kilometers in diameter.

    5040 Rabinowitz, provisional designation 1972 RF, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered by Dutch–American astronomer Tom Gehrels at Palomar Observatory on 15 September 1972. Contrary to most of his discoveries, this asteroid is unrelated to the Palomar–Leiden survey and exclusively credited to Tom Gehrels.

    2074 Shoemaker, provisional designation 1974 UA, is a stony Hungaria asteroid, Mars-crosser and suspected synchronous binary system from the innermost regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 17 October 1974, by astronomer Eleanor Helin at the Palomar Observatory. She named it after American astronomer Eugene Shoemaker.

    4085 Weir, provisional designation 1985 JR, is a stony Eunomian asteroid from the central regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 13 May 1985, by astronomer Carolyn Shoemaker at the Palomar Observatory in California, United States. The asteroid was named after American geologist Doris Blackman Weir.

    12838 Adamsmith, provisional designation 1997 EL55, is a stony Koronis asteroid from the outer region of the asteroid belt, approximately 6 kilometers in diameter. The asteroid was discovered on 9 March 1997, by Belgian astronomer Eric Walter Elst at ESO's La Silla Observatory in northern Chile. It was named after Scottish philosopher and economist Adam Smith.

    52266 Van Flandern is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 10 January 1986, by American astronomers Carolyn and Eugene Shoemaker at the Palomar Observatory in California, United States. The asteroid was later named for American astronomer Tom Van Flandern.

    References

    1. 1 2 3 4 5 "JPL Small-Body Database Browser: 9564 Jeffwynn (1987 SG3)" (2017-03-14 last obs.). Jet Propulsion Laboratory . Retrieved 22 June 2017.
    2. 1 2 3 Schmadel, Lutz D. (2007). "(9564) Jeffwynn". Dictionary of Minor Planet Names – (9564) Jeffwynn. Springer Berlin Heidelberg. p. 699. doi:10.1007/978-3-540-29925-7_7587. ISBN   978-3-540-00238-3.
    3. 1 2 3 4 5 6 7 "LCDB Data for (9564) Jeffwynn". Asteroid Lightcurve Database (LCDB). Retrieved 29 July 2016.
    4. 1 2 Warner, Brian D. (January 2013). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2012 June - September". The Minor Planet Bulletin. 40 (1): 26–29. Bibcode:2013MPBu...40...26W. ISSN   1052-8091 . Retrieved 1 January 2016.
    5. 1 2 3 Carry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry". Icarus. 268: 340–354. arXiv: 1601.02087 . Bibcode:2016Icar..268..340C. doi:10.1016/j.icarus.2015.12.047 . Retrieved 29 July 2016.
    6. Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: 1506.00762 . Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007 . Retrieved 29 July 2016.
    7. 1 2 "9564 Jeffwynn (1987 SG3)". Minor Planet Center. Retrieved 29 July 2016.
    8. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 29 July 2016.