.png) A three-dimensional model of 115 Thyra based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | James Craig Watson |
| Discovery date | 6 August 1871 |
| Designations | |
| (115) Thyra | |
| Pronunciation | /ˈθaɪərə/ [1] |
Named after | Thyra |
| A871 PA | |
| Main belt | |
| Orbital characteristics [2] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 143.31 yr (52344 d) |
| Aphelion | 2.8376 AU (424.50 Gm) |
| Perihelion | 1.92394 AU (287.817 Gm) |
| 2.38077 AU (356.158 Gm) | |
| Eccentricity | 0.19188 |
| 3.67 yr (1341.8 d) | |
Average
orbital speed | 19.13 km/s |
| 108.401 ° | |
| 0° 16m 5.88s / day | |
| Inclination | 11.595° |
| 308.901° | |
| 96.946° | |
| Earth MOID | 0.97246 AU (145.478 Gm) |
| Jupiter MOID | 2.63437 AU (394.096 Gm) |
| TJupiter | 3.486 |
| Physical characteristics | |
| Dimensions | 79.83±1.4
km
[2] 79.83 km [3] |
| Mass | 5.3×1017 kg |
Equatorial
surface gravity | 0.0223 m/s2 |
Equatorial
escape velocity | 0.0422 km/s |
| 7.241 h (0.3017 d) | |
| 0.2747±0.010
[2] 0.275 [3] | |
| Temperature | ~180 K |
| S [4] | |
| 7.51 [2] [3] | |
115 Thyra is a fairly large and bright inner main-belt asteroid that was discovered by Canadian-American astronomer J. C. Watson on August 6, 1871 [5] and was named for Thyra, the consort of King Gorm the Old of Denmark. Based upon its spectrum, it is categorized as a stony S-type asteroid. [6]
Observations made between 1978 and 1981 produced a composite light curve with two minima and maxima. However, a subsequent study in 1983 only found a single minima and maxima. A synodical rotation period of 7.241 hours was determined. This was confirmed by observations between 1995 and 2000. The changes in brightness and color indicate a surface with an uneven composition. [7]
The asteroid has a slightly elongated shape, with a ratio of 1.20 between the lengths of the major and minor axes. The orbital longitude and latitude of the asteroid pole in degrees is estimated to be (λ0, β0) = (68°, 23°). [8] Measurements of the thermal inertia of 115 Thyra give a value of around 75 m−2 K−1 s−1/2, compared to 50 for lunar regolith and 400 for coarse sand in an atmosphere. [3]
- ^ From 'Tyra', a variant of the name.
- ^ a b c d Yeomans, Donald K., "115 Thyra", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
- ^ a b c d Delbo', Marco; Tanga, Paolo (February 2009), "Thermal inertia of main belt asteroids smaller than 100 km from IRAS data", Planetary and Space Science, 57 (2): 259–265, arXiv: 0808.0869, Bibcode: 2009P&SS...57..259D, doi: 10.1016/j.pss.2008.06.015, S2CID 14517561.
- ^ * JPL Small-Body Database Browser
- ^ "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
- ^ DeMeo, Francesca E.; et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus, 202 (1): 160–180, Bibcode: 2009Icar..202..160D, doi: 10.1016/j.icarus.2009.02.005, archived from the original (PDF) on 17 March 2014, retrieved 8 April 2013. See appendix A.
- ^ Michałowski, T.; et al. (March 2004), "Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona", Astronomy and Astrophysics, 416: 353–366, Bibcode: 2004A&A...416..353M, doi: 10.1051/0004-6361:20031706.
- ^ Kryszczyńska, A.; et al. (December 2007), "New findings on asteroid spin-vector distributions", Icarus, 192 (1): 223–237, Bibcode: 2007Icar..192..223K, doi: 10.1016/j.icarus.2007.06.008.
- 115 Thyra at AstDyS-2, Asteroids—Dynamic Site
- 115 Thyra at the JPL Small-Body Database
|
A three-dimensional model of 115 Thyra based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | James Craig Watson |
| Discovery date | 6 August 1871 |
| Designations | |
| (115) Thyra | |
| Pronunciation | /ˈθaɪərə/ [1] |
Named after | Thyra |
| A871 PA | |
| Main belt | |
| Orbital characteristics [2] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 143.31 yr (52344 d) |
| Aphelion | 2.8376 AU (424.50 Gm) |
| Perihelion | 1.92394 AU (287.817 Gm) |
| 2.38077 AU (356.158 Gm) | |
| Eccentricity | 0.19188 |
| 3.67 yr (1341.8 d) | |
Average
orbital speed | 19.13 km/s |
| 108.401 ° | |
| 0° 16m 5.88s / day | |
| Inclination | 11.595° |
| 308.901° | |
| 96.946° | |
| Earth MOID | 0.97246 AU (145.478 Gm) |
| Jupiter MOID | 2.63437 AU (394.096 Gm) |
| TJupiter | 3.486 |
| Physical characteristics | |
| Dimensions | 79.83±1.4
km
[2] 79.83 km [3] |
| Mass | 5.3×1017 kg |
Equatorial
surface gravity | 0.0223 m/s2 |
Equatorial
escape velocity | 0.0422 km/s |
| 7.241 h (0.3017 d) | |
| 0.2747±0.010
[2] 0.275 [3] | |
| Temperature | ~180 K |
| S [4] | |
| 7.51 [2] [3] | |
115 Thyra is a fairly large and bright inner main-belt asteroid that was discovered by Canadian-American astronomer J. C. Watson on August 6, 1871 [5] and was named for Thyra, the consort of King Gorm the Old of Denmark. Based upon its spectrum, it is categorized as a stony S-type asteroid. [6]
Observations made between 1978 and 1981 produced a composite light curve with two minima and maxima. However, a subsequent study in 1983 only found a single minima and maxima. A synodical rotation period of 7.241 hours was determined. This was confirmed by observations between 1995 and 2000. The changes in brightness and color indicate a surface with an uneven composition. [7]
The asteroid has a slightly elongated shape, with a ratio of 1.20 between the lengths of the major and minor axes. The orbital longitude and latitude of the asteroid pole in degrees is estimated to be (λ0, β0) = (68°, 23°). [8] Measurements of the thermal inertia of 115 Thyra give a value of around 75 m−2 K−1 s−1/2, compared to 50 for lunar regolith and 400 for coarse sand in an atmosphere. [3]
- ^ From 'Tyra', a variant of the name.
- ^ a b c d Yeomans, Donald K., "115 Thyra", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
- ^ a b c d Delbo', Marco; Tanga, Paolo (February 2009), "Thermal inertia of main belt asteroids smaller than 100 km from IRAS data", Planetary and Space Science, 57 (2): 259–265, arXiv: 0808.0869, Bibcode: 2009P&SS...57..259D, doi: 10.1016/j.pss.2008.06.015, S2CID 14517561.
- ^ * JPL Small-Body Database Browser
- ^ "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
- ^ DeMeo, Francesca E.; et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus, 202 (1): 160–180, Bibcode: 2009Icar..202..160D, doi: 10.1016/j.icarus.2009.02.005, archived from the original (PDF) on 17 March 2014, retrieved 8 April 2013. See appendix A.
- ^ Michałowski, T.; et al. (March 2004), "Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona", Astronomy and Astrophysics, 416: 353–366, Bibcode: 2004A&A...416..353M, doi: 10.1051/0004-6361:20031706.
- ^ Kryszczyńska, A.; et al. (December 2007), "New findings on asteroid spin-vector distributions", Icarus, 192 (1): 223–237, Bibcode: 2007Icar..192..223K, doi: 10.1016/j.icarus.2007.06.008.
- 115 Thyra at AstDyS-2, Asteroids—Dynamic Site
- 115 Thyra at the JPL Small-Body Database