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1425 Tuorla
Discovery [1]
Discovered by K. Inkeri
Discovery site Turku Obs.
Discovery date3 April 1937
Designations
(1425) Tuorla
Named after
 Tuorla Observatory [2]
(Inst. for Astronomy and Optics)
1937 GB · 1950 KC
1950 LQ
main-belt · ( middle)
Eunomia [3] [4]
Orbital characteristics [1]
Epoch 4 September 2017 ( JD 2458000.5)
Uncertainty parameter 0
Observation arc67.14 yr (24,522 days)
Aphelion2.8766 AU
Perihelion2.3483 AU
2.6125 AU
Eccentricity0.1011
4.22 yr (1,542 days)
40.218 °
0° 14m 0.24s / day
Inclination12.975°
185.99°
342.25°
Physical characteristics
Dimensions11.795±0.874 km [5]
14.34±1.08 km [6]
14.94±1.1 km [3] [7]
6.76±0.01 h [a]
6.97±0.01 h [8]
7.748±0.0027 h [9]
7.75±0.06 h [10]
0.2389 (derived) [3]
0.2390±0.040 [7]
0.260±0.041 [6]
0.383±0.083 [5]
S [3] [11]
11.173±0.003 (R) [9] · 11.30 [3] [5] [6] [7] · 11.4 [1] · 11.91±0.41 [11]

1425 Tuorla, provisional designation 1937 GB, is a stony Eunomian asteroid from the central regions of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 3 April 1937, by Finnish astronomer Kustaa Inkeri at the Iso-Heikkilä Observatory in Turku, southwestern Finland. [12] The asteroid was named after the Tuorla Observatory of the University of Turku. [2] It was Kustaa Inkeri's only asteroid discovery. [13]

Orbit and classification

Tuorla is a member of the Eunomia family ( 502), [3] [4] a prominent family of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members. [14]: 23  It orbits the Sun at a distance of 2.3–2.9  AU once every 4 years and 3 months (1,542 days). Its orbit has an eccentricity of 0.10 and an inclination of 13 ° with respect to the ecliptic. [1] The body's observation arc begins at Turku, the night before its official discovery observation. [12]

Physical characteristics

Tuorla has been characterized as a stony S-type asteroid by Pan-STARRS photometric survey, [11] in accordance with the overall spectral type for members of the Eunomia family. [14]: 23 

Rotation period

In April 2013, the so-far best-rated a rotational lightcurve of Tuorla was obtained from photometric observations by astronomer Vladimir Benishek at Belgrade Observatory in Serbia. Lightcurve analysis gave a well-defined rotation period of 7.75 hours (h) with a brightness variation of 0.24 magnitude ( U=3). [10] Other lightcurves were obtained by Alfonso Carreno Garceran (6.76 h), [a] Laurent Bernasconi (7.75 h), [8] and the Palomar Transient Factory (7.748 h), [9]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Tuorla measures between 11.795 and 14.94 kilometers in diameter and its surface has an albedo between 0.2390 and 0.383. [5] [6] [7] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2389 and adopts a diameter of 14.94 kilometers from IRAS, based on an absolute magnitude of 11.3. [3]

Naming

This minor planet was named after the Tuorla Observatory, the Research Institute for Astronomy and Optics, of the University of Turku, located in Piikkiö near Turku, Finland. [2] The Tuorla Observatory was established by prolific minor-planet discoverer Yrjö Väisälä in 1952, as an alternative to the Iso-Heikkilä Observatory, where this asteroid was discovered. The official naming citation was published by the Minor Planet Center on 30 January 1964 ( M.P.C. 2277). [15]

Notes

  1. ^ a b Garceran (2013) web: rotation period hours with a brightness amplitude of mag. Summary figures for (1425) Tuorla at LCDB

References

  1. ^ a b c d "JPL Small-Body Database Browser: 1425 Tuorla (1937 GB)" (2017-07-05 last obs.). Jet Propulsion Laboratory. Archived from the original on 18 September 2020. Retrieved 26 October 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). "(1425) Tuorla". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 114. doi: 10.1007/978-3-540-29925-7_1426. ISBN  978-3-540-00238-3.
  3. ^ a b c d e f g "LCDB Data for (1425) Tuorla". Asteroid Lightcurve Database (LCDB). Retrieved 26 October 2017.
  4. ^ a b "Asteroid 1425 Tuorla – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
  5. ^ a b c d 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. Retrieved 26 October 2017.
  6. ^ a b c d 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)
  7. ^ a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. Retrieved 17 October 2019.
  8. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1425) Tuorla". Geneva Observatory. Retrieved 26 October 2017.
  9. ^ a b c Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv: 1504.04041. Bibcode: 2015AJ....150...75W. doi: 10.1088/0004-6256/150/3/75. Retrieved 26 October 2017.
  10. ^ a b Benishek, Vladimir (April 2014). "Rotation Period Determination for 1425 Tuorla, 1468 Zomba, 1486 Marilyn, 2112 Ulyanov, and (101158) 2000 OL". The Minor Planet Bulletin. 41 (2): 126–127. Bibcode: 2014MPBu...41..126B. ISSN  1052-8091. Retrieved 26 October 2017.
  11. ^ a b c 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 26 October 2017.
  12. ^ a b "1425 Tuorla (1937 GB)". Minor Planet Center. Retrieved 26 October 2017.
  13. ^ "Minor Planet Discoverers (by number)". Minor Planet Center. 5 October 2017. Retrieved 26 October 2017.
  14. ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv: 1502.01628. Bibcode: 2015aste.book..297N. doi: 10.2458/azu_uapress_9780816532131-ch016. ISBN  9780816532131.
  15. ^ Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p.  221. doi: 10.1007/978-3-642-01965-4. ISBN  978-3-642-01964-7.

External links

Retrieved from " https://en.wikipedia.org/?title=1425_Tuorla&oldid=1191752830"
From Wikipedia, the free encyclopedia

1425 Tuorla
Discovery [1]
Discovered by K. Inkeri
Discovery site Turku Obs.
Discovery date3 April 1937
Designations
(1425) Tuorla
Named after
 Tuorla Observatory [2]
(Inst. for Astronomy and Optics)
1937 GB · 1950 KC
1950 LQ
main-belt · ( middle)
Eunomia [3] [4]
Orbital characteristics [1]
Epoch 4 September 2017 ( JD 2458000.5)
Uncertainty parameter 0
Observation arc67.14 yr (24,522 days)
Aphelion2.8766 AU
Perihelion2.3483 AU
2.6125 AU
Eccentricity0.1011
4.22 yr (1,542 days)
40.218 °
0° 14m 0.24s / day
Inclination12.975°
185.99°
342.25°
Physical characteristics
Dimensions11.795±0.874 km [5]
14.34±1.08 km [6]
14.94±1.1 km [3] [7]
6.76±0.01 h [a]
6.97±0.01 h [8]
7.748±0.0027 h [9]
7.75±0.06 h [10]
0.2389 (derived) [3]
0.2390±0.040 [7]
0.260±0.041 [6]
0.383±0.083 [5]
S [3] [11]
11.173±0.003 (R) [9] · 11.30 [3] [5] [6] [7] · 11.4 [1] · 11.91±0.41 [11]

1425 Tuorla, provisional designation 1937 GB, is a stony Eunomian asteroid from the central regions of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 3 April 1937, by Finnish astronomer Kustaa Inkeri at the Iso-Heikkilä Observatory in Turku, southwestern Finland. [12] The asteroid was named after the Tuorla Observatory of the University of Turku. [2] It was Kustaa Inkeri's only asteroid discovery. [13]

Orbit and classification

Tuorla is a member of the Eunomia family ( 502), [3] [4] a prominent family of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members. [14]: 23  It orbits the Sun at a distance of 2.3–2.9  AU once every 4 years and 3 months (1,542 days). Its orbit has an eccentricity of 0.10 and an inclination of 13 ° with respect to the ecliptic. [1] The body's observation arc begins at Turku, the night before its official discovery observation. [12]

Physical characteristics

Tuorla has been characterized as a stony S-type asteroid by Pan-STARRS photometric survey, [11] in accordance with the overall spectral type for members of the Eunomia family. [14]: 23 

Rotation period

In April 2013, the so-far best-rated a rotational lightcurve of Tuorla was obtained from photometric observations by astronomer Vladimir Benishek at Belgrade Observatory in Serbia. Lightcurve analysis gave a well-defined rotation period of 7.75 hours (h) with a brightness variation of 0.24 magnitude ( U=3). [10] Other lightcurves were obtained by Alfonso Carreno Garceran (6.76 h), [a] Laurent Bernasconi (7.75 h), [8] and the Palomar Transient Factory (7.748 h), [9]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Tuorla measures between 11.795 and 14.94 kilometers in diameter and its surface has an albedo between 0.2390 and 0.383. [5] [6] [7] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2389 and adopts a diameter of 14.94 kilometers from IRAS, based on an absolute magnitude of 11.3. [3]

Naming

This minor planet was named after the Tuorla Observatory, the Research Institute for Astronomy and Optics, of the University of Turku, located in Piikkiö near Turku, Finland. [2] The Tuorla Observatory was established by prolific minor-planet discoverer Yrjö Väisälä in 1952, as an alternative to the Iso-Heikkilä Observatory, where this asteroid was discovered. The official naming citation was published by the Minor Planet Center on 30 January 1964 ( M.P.C. 2277). [15]

Notes

  1. ^ a b Garceran (2013) web: rotation period hours with a brightness amplitude of mag. Summary figures for (1425) Tuorla at LCDB

References

  1. ^ a b c d "JPL Small-Body Database Browser: 1425 Tuorla (1937 GB)" (2017-07-05 last obs.). Jet Propulsion Laboratory. Archived from the original on 18 September 2020. Retrieved 26 October 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). "(1425) Tuorla". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 114. doi: 10.1007/978-3-540-29925-7_1426. ISBN  978-3-540-00238-3.
  3. ^ a b c d e f g "LCDB Data for (1425) Tuorla". Asteroid Lightcurve Database (LCDB). Retrieved 26 October 2017.
  4. ^ a b "Asteroid 1425 Tuorla – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
  5. ^ a b c d 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. Retrieved 26 October 2017.
  6. ^ a b c d 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)
  7. ^ a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. Retrieved 17 October 2019.
  8. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1425) Tuorla". Geneva Observatory. Retrieved 26 October 2017.
  9. ^ a b c Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv: 1504.04041. Bibcode: 2015AJ....150...75W. doi: 10.1088/0004-6256/150/3/75. Retrieved 26 October 2017.
  10. ^ a b Benishek, Vladimir (April 2014). "Rotation Period Determination for 1425 Tuorla, 1468 Zomba, 1486 Marilyn, 2112 Ulyanov, and (101158) 2000 OL". The Minor Planet Bulletin. 41 (2): 126–127. Bibcode: 2014MPBu...41..126B. ISSN  1052-8091. Retrieved 26 October 2017.
  11. ^ a b c 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 26 October 2017.
  12. ^ a b "1425 Tuorla (1937 GB)". Minor Planet Center. Retrieved 26 October 2017.
  13. ^ "Minor Planet Discoverers (by number)". Minor Planet Center. 5 October 2017. Retrieved 26 October 2017.
  14. ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv: 1502.01628. Bibcode: 2015aste.book..297N. doi: 10.2458/azu_uapress_9780816532131-ch016. ISBN  9780816532131.
  15. ^ Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p.  221. doi: 10.1007/978-3-642-01965-4. ISBN  978-3-642-01964-7.

External links

Retrieved from " https://en.wikipedia.org/?title=1425_Tuorla&oldid=1191752830"

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