115 Thyra: Difference between revisions

115 Thyra
	A three-dimensional model of 115 Thyra based on its light curve.
Discovery
Discovered by	James Craig Watson
Discovery date	6 August 1871
Designations
MPC designation	(115) Thyra
Pronunciation	/ˈθaɪərə/
Named after	Thyra
Alternative designations	A871 PA
Minor planet category	Main belt
Orbital characteristics
	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)
Semi-major axis	2.38077 AU (356.158 Gm)
Eccentricity	0.19188
Orbital period (sidereal)	3.67 yr (1341.8 d)
Average orbital speed	19.13 km/s
Mean anomaly	108.401°
Mean motion	0° 16m 5.88s / day
Inclination	11.595°
Longitude of ascending node	308.901°
Argument of perihelion	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; 79.83 km
Mass	5.3×1017 kg
Equatorial surface gravity	0.0223 m/s2
Equatorial escape velocity	0.0422 km/s
Synodic rotation period	7.241 h (0.3017 d)
Geometric albedo	0.2747±0.010; 0.275
Temperature	~180 K
Spectral type	S
Absolute magnitude (H)	7.51

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Latest revision as of 19:44, 25 December 2023

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]

References

^ 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.

External links

115 Thyra at AstDyS-2, Asteroids—Dynamic Site
- Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
115 Thyra at the JPL Small-Body Database
- Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters

[1] From 'Tyra', a variant of the name.

[JPL-2] Yeomans, Donald K., "115 Thyra", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.

[Delbo2009-3] 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.

[4] *JPL Small-Body Database Browser

[IAU_MPC-5] "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.

[DeMeo2009-6] 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.

[Michalowski2004-7] 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.

[Kryszczynska2007-8] 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.

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[2]

[3]

[4]

[5]

[6]

[7]

[8]

@@ Line 1: / Line 1: @@
+{{Short description|Main-belt asteroid}}
+{{Use dmy dates|date=October 2019}}
 {{Infobox planet
  | minorplanet=yes
@@ Line 8: / Line 10: @@
  | discovered=6 August 1871
  | mpc_name=(115) Thyra
- | alt_names=
+ | alt_names=A871 PA
- | pronounced={{IPAc-en|'|θ|aɪ|r|ə}}
+ | pronounced={{IPAc-en|'|θ|aɪər|ə}}<ref>From 'Tyra', a variant of the name.</ref>
  | named_after=[[Thyra]]
  | mp_category=[[Main belt]]
@@ Line 27: / Line 29: @@
  | mass=5.3{{e|17}} kg
  | density=<!-- ? g/cm³ -->
- | surface_grav=0.0223 m/s²
+ | surface_grav=0.0223 m/s<sup>2</sup>
  | escape_velocity=0.0422 km/s
  | rotation={{Convert|7.241|h|d|abbr=on|lk=on}}
- | spectral_type=[[S-type asteroid|S]]<ref>*[http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=115 JPL Small-Body Database Browser<!-- Bot generated title -->]</ref>
+ | spectral_type=[[S-type asteroid|S]]<ref>*[https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=115 JPL Small-Body Database Browser<!-- Bot generated title -->]</ref>
  | abs_magnitude=7.51<ref name="JPL"/><ref name="Delbo2009"/>
  | albedo={{val|0.2747|0.010}}<ref name="JPL"/><br />0.275<ref name="Delbo2009"/>
@@ Line 42: / Line 44: @@
 }}
-'''Thyra''' ([[minor planet designation]]: '''115 Thyra''') is a fairly large and bright inner [[main-belt]] [[asteroid]] that was discovered by Canadian-American astronomer [[James Craig Watson|J. C. Watson]] on August 6, 1871<ref name="IAU_MPC"/> 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]].<ref name="DeMeo2009"/>
+'''115 Thyra''' is a fairly large and bright inner [[main-belt]] [[asteroid]] that was discovered by Canadian-American astronomer [[James Craig Watson|J. C. Watson]] on August 6, 1871<ref name="IAU_MPC"/> 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]].<ref name="DeMeo2009"/>
 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.<ref name="Michalowski2004"/>
@@ Line 75: / Line 77: @@
  | first2    = Paolo
  | title     = Thermal inertia of main belt asteroids smaller than 100 km from IRAS data
- | work      = Planetary and Space Science
+ | journal      = Planetary and Space Science
  | volume    = 57
  | issue     = 2
@@ Line 83: / Line 85: @@
  | bibcode   = 2009P&SS...57..259D
  | postscript= .
-|arxiv = 0808.0869 }}</ref>
+|arxiv = 0808.0869 | s2cid = 14517561
+ }}</ref>
 <ref name="Michalowski2004">{{Citation
@@ Line 110: / Line 113: @@
  | display-authors = 1
  | title     = Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona
- | work      = Astronomy and Astrophysics
+ | journal      = Astronomy and Astrophysics
  | volume    = 416
  | pages     = 353–366
@@ Line 116: / Line 119: @@
  | doi       = 10.1051/0004-6361:20031706
  | bibcode   = 2004A&A...416..353M
- | postscript= .}}</ref>
+ | postscript= .| doi-access= free
+ }}</ref>
 <ref name="Kryszczynska2007">{{Citation
@@ Line 133: / Line 137: @@
  | display-authors = 1
  | title     = New findings on asteroid spin-vector distributions
- | work      = Icarus
+ | journal      = Icarus
  | volume    = 192
  | pages     = 223–237
  |date=December 2007
+ | issue = 1
  | doi       = 10.1016/j.icarus.2007.06.008
  | bibcode   = 2007Icar..192..223K
@@ Line 152: / Line 157: @@
  |display-authors = 1
  |title           = An extension of the Bus asteroid taxonomy into the near-infrared
- |work            = Icarus
+ |journal            = Icarus
  |volume          = 202
  |issue           = 1
@@ Line 162: / Line 167: @@
  |accessdate      = 2013-04-08
  |postscript      = .
- |deadurl         = yes
+ |url-status         = dead
  |archiveurl      = https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf
  |archivedate     = 2014-03-17
- |df              = }} See appendix A.</ref>
+ }} See appendix A.</ref>
 }} <!-- end of reflist -->
@@ Line 175: / Line 180: @@
 {{Minor planets navigator |114 Kassandra |number=115 |116 Sirona}}
 {{Small Solar System bodies}}
+{{Authority control}}
 {{DEFAULTSORT:Thyra}}
 [[Category:Background asteroids|000115]]
-[[Category:Numbered minor planets|000115]]
+[[Category:Discoveries by James Craig Watson]]
-[[Category:Discoveries by James Watson]]
-[[Category:Minor planets named for people]]
 [[Category:Named minor planets]]
 [[Category:S-type asteroids (SMASS)|000115]]