| Discovery [1] | |
|---|---|
| Discovered by | S. Belyavskyj |
| Discovery site | Simeiz Obs. |
| Discovery date | 5 November 1921 |
| Designations | |
| (969) Leocadia | |
| Pronunciation | /liːoʊˈkeɪdiə/ [2] |
Named after | unknown [3] |
| A921 VC · 1940 RV 1944 SB · 1948 UG 1963 PA · 1921 KZ | |
|
main-belt
[1]
[4] · (
inner) background [5] [6] | |
| Orbital characteristics [4] | |
| Epoch 31 May 2020 ( JD 2459000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 98.12 yr (35,837 d) |
| Aphelion | 2.9694 AU |
| Perihelion | 1.9537 AU |
| 2.4615 AU | |
| Eccentricity | 0.2063 |
| 3.86 yr (1,411 d) | |
| 199.53 ° | |
| 0° 15m 18.72s / day | |
| Inclination | 2.2928° |
| 287.76° | |
| 91.332° | |
| Physical characteristics | |
| 6.87±0.01 h [10] [11] | |
| 12.8 [1] [4] | |
969 Leocadia ( prov. designation: A921 VC or 1921 KZ) is a very dark background asteroid from the inner regions of the asteroid belt, approximately 19 kilometers (12 miles) in diameter. It was discovered on 5 November 1921, by Russian astronomer Sergey Belyavsky at the Simeiz Observatory on the Crimean peninsula. [1] The uncommon F-type asteroid (FX) has a rotation period of 6.9 hours and is likely regular in shape. [10] Any reference of the asteroid's name to a person is unknown. [3]
Leocadia is a non- family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. [5] [6] It orbits the Sun in the inner main-belt at a distance of 2.0–3.0 AU once every 3 years and 10 months (1,411 days; semi-major axis of 2.46 AU). Its orbit has an eccentricity of 0.21 and an inclination of 2 ° with respect to the ecliptic. [4] The body's observation arc begins at Uccle Observatory in February 1933, more than a decade after its official discovery observation Simeiz Observatory on 5 November 1921. [1]
This minor planet is named after a Feminine Russian first name. Any reference of this name to a person or occurrence is unknown. [3]
Among the many thousands of named minor planets, Leocadia is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 Eva and 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth. [12]
In the Tholen classification (FXU:), Leocadia is an uncommon and dark F-type asteroid, somewhat similar to that of an X-type, though with an unusual (U) and noisy (:) spectra. [4]
In December 2006, a rotational lightcurve of Leocadia was obtained from photometric observations by Italian amateur astronomers Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station ( A12). Lightcurve analysis gave a rotation period of 6.87±0.01 hours with a brightness amplitude of 0.14±0.01 magnitude ( U=2), which is indicative of a rather spherical, non-irregular shape. [10] [11]
According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Japanese Akari satellite, and the Infrared Astronomical Satellite IRAS, Leocadia measures 17.321±0.218, 19.37±0.22 and 19.51±0.7 kilometers in diameter, and its surface has a very low albedo of 0.019±0.005, 0.0435±0.003 and 0.045±0.001, respectively. [7] [8] [9] Additional measurements by the WISE telescope were published giving a mean diameter as low as 13.58±3.09 km. [11] The Collaborative Asteroid Lightcurve Link adopts the result from IRAS, that is, an albedo of 0.0435 and a diameter of 19.51 kilometers based on an absolute magnitude of 9.22. [11]
An asteroid occultation on 19 August 2013, gave a best-fit ellipse dimension of 19.0 × 19.0 kilometers. [6] These timed observations are taken when the asteroid passes in front of a distant star. However the measurements for Leocadia were of poor quality. [6]
- ^ a b c d e "969 Leocadia (A921 VC)". Minor Planet Center. Retrieved 11 February 2020.
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ a b c Schmadel, Lutz D. (2007). "(969) Leocadia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 85. doi: 10.1007/978-3-540-29925-7_970. ISBN 978-3-540-00238-3.
- ^ a b c d e f g h "JPL Small-Body Database Browser: 969 Leocadia (A921 VC)" (2020-01-07 last obs.). Jet Propulsion Laboratory. Retrieved 11 February 2020.
- ^ a b "Asteroid 969 Leocadia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 11 February 2020.
- ^ a b c d "Asteroid 969 Leocadia". Small Bodies Data Ferret. Retrieved 11 February 2020.
- ^ a b c Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv: 1209.5794. Bibcode: 2012ApJ...759L...8M. doi: 10.1088/2041-8205/759/1/L8.
- ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode: 2011PASJ...63.1117U. doi: 10.1093/pasj/63.5.1117. ( online, AcuA catalog p. 153)
- ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. Retrieved 11 February 2020.
- ^ a b c Behrend, Raoul. "Asteroids and comets rotation curves – (969) Leocadia". Geneva Observatory. Retrieved 11 February 2020.
- ^ a b c d "LCDB Data for (969) Leocadia". Asteroid Lightcurve Database (LCDB). Retrieved 11 February 2020.
- ^ Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning". Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929. ISBN 978-3-540-00238-3.
- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 969 Leocadia at AstDyS-2, Asteroids—Dynamic Site
- 969 Leocadia at the JPL Small-Body Database
| Discovery [1] | |
|---|---|
| Discovered by | S. Belyavskyj |
| Discovery site | Simeiz Obs. |
| Discovery date | 5 November 1921 |
| Designations | |
| (969) Leocadia | |
| Pronunciation | /liːoʊˈkeɪdiə/ [2] |
Named after | unknown [3] |
| A921 VC · 1940 RV 1944 SB · 1948 UG 1963 PA · 1921 KZ | |
|
main-belt
[1]
[4] · (
inner) background [5] [6] | |
| Orbital characteristics [4] | |
| Epoch 31 May 2020 ( JD 2459000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 98.12 yr (35,837 d) |
| Aphelion | 2.9694 AU |
| Perihelion | 1.9537 AU |
| 2.4615 AU | |
| Eccentricity | 0.2063 |
| 3.86 yr (1,411 d) | |
| 199.53 ° | |
| 0° 15m 18.72s / day | |
| Inclination | 2.2928° |
| 287.76° | |
| 91.332° | |
| Physical characteristics | |
| 6.87±0.01 h [10] [11] | |
| 12.8 [1] [4] | |
969 Leocadia ( prov. designation: A921 VC or 1921 KZ) is a very dark background asteroid from the inner regions of the asteroid belt, approximately 19 kilometers (12 miles) in diameter. It was discovered on 5 November 1921, by Russian astronomer Sergey Belyavsky at the Simeiz Observatory on the Crimean peninsula. [1] The uncommon F-type asteroid (FX) has a rotation period of 6.9 hours and is likely regular in shape. [10] Any reference of the asteroid's name to a person is unknown. [3]
Leocadia is a non- family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. [5] [6] It orbits the Sun in the inner main-belt at a distance of 2.0–3.0 AU once every 3 years and 10 months (1,411 days; semi-major axis of 2.46 AU). Its orbit has an eccentricity of 0.21 and an inclination of 2 ° with respect to the ecliptic. [4] The body's observation arc begins at Uccle Observatory in February 1933, more than a decade after its official discovery observation Simeiz Observatory on 5 November 1921. [1]
This minor planet is named after a Feminine Russian first name. Any reference of this name to a person or occurrence is unknown. [3]
Among the many thousands of named minor planets, Leocadia is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 Eva and 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth. [12]
In the Tholen classification (FXU:), Leocadia is an uncommon and dark F-type asteroid, somewhat similar to that of an X-type, though with an unusual (U) and noisy (:) spectra. [4]
In December 2006, a rotational lightcurve of Leocadia was obtained from photometric observations by Italian amateur astronomers Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station ( A12). Lightcurve analysis gave a rotation period of 6.87±0.01 hours with a brightness amplitude of 0.14±0.01 magnitude ( U=2), which is indicative of a rather spherical, non-irregular shape. [10] [11]
According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Japanese Akari satellite, and the Infrared Astronomical Satellite IRAS, Leocadia measures 17.321±0.218, 19.37±0.22 and 19.51±0.7 kilometers in diameter, and its surface has a very low albedo of 0.019±0.005, 0.0435±0.003 and 0.045±0.001, respectively. [7] [8] [9] Additional measurements by the WISE telescope were published giving a mean diameter as low as 13.58±3.09 km. [11] The Collaborative Asteroid Lightcurve Link adopts the result from IRAS, that is, an albedo of 0.0435 and a diameter of 19.51 kilometers based on an absolute magnitude of 9.22. [11]
An asteroid occultation on 19 August 2013, gave a best-fit ellipse dimension of 19.0 × 19.0 kilometers. [6] These timed observations are taken when the asteroid passes in front of a distant star. However the measurements for Leocadia were of poor quality. [6]
- ^ a b c d e "969 Leocadia (A921 VC)". Minor Planet Center. Retrieved 11 February 2020.
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ a b c Schmadel, Lutz D. (2007). "(969) Leocadia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 85. doi: 10.1007/978-3-540-29925-7_970. ISBN 978-3-540-00238-3.
- ^ a b c d e f g h "JPL Small-Body Database Browser: 969 Leocadia (A921 VC)" (2020-01-07 last obs.). Jet Propulsion Laboratory. Retrieved 11 February 2020.
- ^ a b "Asteroid 969 Leocadia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 11 February 2020.
- ^ a b c d "Asteroid 969 Leocadia". Small Bodies Data Ferret. Retrieved 11 February 2020.
- ^ a b c Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv: 1209.5794. Bibcode: 2012ApJ...759L...8M. doi: 10.1088/2041-8205/759/1/L8.
- ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode: 2011PASJ...63.1117U. doi: 10.1093/pasj/63.5.1117. ( online, AcuA catalog p. 153)
- ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. Retrieved 11 February 2020.
- ^ a b c Behrend, Raoul. "Asteroids and comets rotation curves – (969) Leocadia". Geneva Observatory. Retrieved 11 February 2020.
- ^ a b c d "LCDB Data for (969) Leocadia". Asteroid Lightcurve Database (LCDB). Retrieved 11 February 2020.
- ^ Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning". Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929. ISBN 978-3-540-00238-3.
- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 969 Leocadia at AstDyS-2, Asteroids—Dynamic Site
- 969 Leocadia at the JPL Small-Body Database