博碩士論文 101289003 詳細資訊



以作者查詢圖書館館藏 、以作者查詢臺灣博碩士 、以作者查詢全國書目 、勘誤回報 、線上人數：66 、訪客IP：3.145.16.251
姓名 潘康嫻(Kang-Shian Pan)  查詢紙本館藏   畢業系所 天文研究所
論文名稱 鹿林一米望遠鏡對主帶小行星的光度及偏振觀測分析
(Photometric and Polarimetric Observations of Main Belt Asteroids at Lulin Observatory)
相關論文
★ 土衛六「泰坦」離子球層的化學-動力學模型★ KBOs星體碰撞與生命及行星大氣起源
★ 行星狀星雲形態之多光譜波段觀測★ 木衛一埃歐鈉雲噴流之結構與時間變化
★ 早期太陽系系統中KBOs的形成與碰撞演化★ 彗星2001A2 （LINEAR）的光度觀測
★ SDSS之RR Lyrae候選變星之確認觀測★ 銀河系核心及盤面的隨機恆星形成歷史
★ 宇宙射線中的氦原子核能譜★ 小行星對於地球原始海水的貢獻
★ 行星狀星雲Hα結構之分析★ 在星系團中的相對論性電子和SZ效應
★ 重力透鏡和交互作用星系的資料探勘★ 在疏散星團中尋找系外行星與變星
★ 原恆星吸積盤動態模擬與氣體固態粒子作用初步探討★ 大型EKBO(Quaoar, Ixion, 2004DW)的自轉週期和表面顏色的測量
檔案 [Endnote RIS 格式]    [Bibtex 格式]    [相關文章]   [文章引用]   [完整記錄]   [館藏目錄]   [檢視]  [下載]
  1. 本電子論文使用權限為同意立即開放。
  2. 已達開放權限電子全文僅授權使用者為學術研究之目的，進行個人非營利性質之檢索、閱讀、列印。
  3. 請遵守中華民國著作權法之相關規定，切勿任意重製、散佈、改作、轉貼、播送，以免觸法。

摘要(中) 根據目前的行星形成理論及模型，主帶小行星是由早期太陽系中行星碰撞過程及受行星的重力擾動後的產物，遺留至今保留著許多早期太陽系當時的物質與化學訊息，因此被視為解開太陽系形成與演化的重要線索之一。為了瞭解位於主帶小行星的結構與表面物質等細節，我們使用鹿林天文台的一米可見光望遠鏡(Lulin One-meter Telescope, LOT)，搭配三色成像偏振儀（Triple Range Imager and Polarimeter, TRIPOL）、光度儀器和LISA光譜儀來進行小行星的偏振、光度和光譜觀測。

在論文的第一部份，為了校正及確認三色成像偏振儀在觀測小行星的可靠性，我們利用偏振量與軌道相位角（太陽－小行星－地球之間形成的夾角）的特徵曲線，針對已知分類的小行星做觀測分析，例如富含矽化合物的S型、富含碳質化合物的C型（與相似物質組成的Ch型、B型）、富含鎳鐵金屬的Ｍ型、與富含鈣鋁包裹體的L型。從觀測結果中，我們的結果與前人的偏振觀測成果一致，並且印證三色成像偏振儀可應用於小行星偏振觀測的準確性。接著，我們也利用偏振儀來針對金屬含量高的小行星編號16的賽姬小行星（16 Psyche）做觀測。在雙色指數圖（color-color diagram, g′-r′和r′-i′）和偏振光變曲線的分析結果中，我們發現賽姬小行星的偏振光變曲線較為平坦，因此較不容易將光變曲線與偏振特徵曲線做關聯性。最後，三色成像偏振也可以藉由偏振光變曲線及相位角來找尋，帶有太陽系發現最古老礦物的L型小行星—Barbarians。

論文的第二部分，根據小行星的瓦礫堆模型，我們藉由小行星光變曲線資料庫（Lightcurve Database）、廣角紅外線尋天觀測計畫中的NEOWISE、和小行星家族成員資料庫（Hierachical Clustering Method, HCM），用統計分析比較了S型與C型小行星家族成員的大小、形狀和週期分佈，來研究小行星的組成與結構。在S型和C型小行星的週期分佈比較中，我們的結果顯示S型小行星的自轉週期與先前的研究相符為2.2小時，而C型的小行星的自轉週期極限應修正約為3小時，此結果可以支持兩者不同分類的小行星物質密度不同。此外，我們也觀測了在C型司理小行星家族（Themis family）中的巴索夫小行星（3599 Basov），不同於之前研究C型的小行星的自轉週期極限為3小時，該小行星的自轉週期為2.157±0.037小時，其光譜分析結果，與典型C型小行星的光譜特徵相似，可以作為C型超快自旋小行星的候選者。
摘要(英) The main-belt asteroids provide valuable information for us to study the general history of the solar system since they are considered the leftover planetesimals during the formation and evolution of the planetary disk. In order to understand the role-play of asteroids in planetary system formation, tracing the physical parameters to figure out the actual structures and compositions is one important way. We aim to investigate the albedo, which is related to the composition and structure of asteroids, by multi-method such as 1)polarimetry using the Triple Range Imager and Polarimeter (TRIPOL) instrument, 2) photometry of Charge-coupled device (CCD) instrument, and 3) a spectrum of LISA spectrograph, observations on the Lulin One-meter Telescope (LOT).

In the first part of this thesis, we demonstrated the technical properties and capability of TRIPOL instrument. We observed a number of bright asteroids with known taxonomic classifications at different phase angles, including B-type, C-type, Ch-type, M-type, S-type, and L-type. By measuring polarization degree with phase angle tracing, We confirmed the validity and reliability of the TRIPOL instrument were working. Furthermore, to study the surface texture of a single asteroid, we also measured rotationally resolved photo-polarimetric variation of a metal-rich object (16) Psyche. Our measurements showed no change in the $g′$-$r′$ and $r′$-$i′$ colors of the rotationally resolved photometry and the intriguing variability in the polarization degree as a function of the rotational phase. The TRIPOL instrument can also be used to measure the polarization of the Barbarians with higher phase angles.

In the second part of this thesis, utilizing the Lightcurve database, NEOWISE, and Hierarchical Clustering Method (HCM) datasets, we analyzed to investigate the differences in size, shape, and rotation period distributions among two S-type and C-type asteroid families based on the compositions and the rubble-pile structure model. From the rotation period distributions, we found that the S-type and C-type asteroids have different spin limits, with the S-type period P$_s$ = 2 hours and the C-type period P$_c$ = 3 hours, respectively. That implies the difference in their bulk densities. In addition, we analyzed a sizable C-type super-fast rotator candidate, asteroid (3599) Basov, to look into the rotation period and taxonomic classification through photometry and spectroscopy using the Lulin One-meter Telescope (LOT) at the Lulin Observatory. The rotation period of asterid (3599) Basov was 2.157$pm0.037$ hours, and the result of reflectance spectrum result was similar to typical C-type asteroids.
關鍵字(中) ★ 主帶小行星
★ 偏振
★ 相位角與偏振特徵曲線
★ 超快自旋小行星		 關鍵字(英) ★ Asteroids
★ Polarimetry
★ Phase-polarimetry Curve
★ Super-fast Rotator
論文目次 英文摘要Abstract in English . . . xv
中文摘要Abstract in Chinese . . . xvii
誌謝Acknowledgements . . . xix
List of Figures . . . xxiii
List of Tables . . . xxv
1 Introduction . . . 1
1.1 The origin of main belt asteroids . . . 1
1.2 Observations of main belt asteroids . . . 3
1.2.1 Photometry . . . 3
1.2.1.1 Light curves . . . 3
1.2.1.2 Taxonomy and Albedo . . . 6
1.2.1.3 Phase functions . . . 6
1.2.2 Polarimetry . . . 9
1.2.2.1 Phase-polarimetry curve . . . 10
1.2.2.2 Rotationally resolved polarimetry . . . 13
2 TRIPOL polarization operating of observation . . . 17
2.1 Instrument description . . . 17
2.2 Definition of polarimetric parameters . . . 18
2.3 Assessment of instrumental polarization and stability . . . 20
2.4 Polarimetric observations of asteroids of different taxonomic classes from Lulin . . . 27
2.5 Results . . . 28
2.5.1 B-type asteroids . . . 28
2.5.2 C-class asteroids . . . 29
2.5.3 M-type asteroids . . . 31
2.5.4 S-type asteroids . . . 36
2.6 Discussion . . . 36
2.7 Summary . . . 43
3 TRIPOL polarimetric observing applications . . .45
3.1 Polarimetric Observation of M-type asteroids and Metal-Rich Asteroid (16) Psyche . . . 45
3.1.1 Observation . . . 47
3.1.2 Results . . . 48
3.1.3 Discussion . . . 50
3.1.4 Summary . . . 52
3.2 Looking for the Barbarian asteroids . . . 54
3.2.1 Targets selections & Observation . . . 55
3.2.2 Polarization phase curve . . . 58
3.2.3 Future work . . . 60
4 A Comparison of the C-type and S-type Families: Sizes, Shapes, and Rotation Periods . . . 61
4.1 Introduction . . . 61
4.2 Asteroid families selection . . . 63
4.3 The size frequency distributions . . . 66
4.4 The shape distributions . . . 68
4.5 The rotation period distributions . . . 74
4.6 Potential C-type superfast rotators . . . 76
4.7 Is (3599) Basov a large C-type super-fast rotator? . . . 80
4.7.1 Observation . . . 80
4.7.1.1 Photometry . . . 80
4.7.1.2 Spectroscopy . . . 81
4.7.2 Data Analysis and Result . . . 81
4.7.2.1 Rotation period . . . 81
4.7.2.2 Taxonomic classification . . . 86
4.7.3 Discussion . . . 86
4.8 Summary . . . 88
5 Summary . . . 99
Bibliography . . . 103
Appendix . . . 125
參考文獻 1. S. Aljbaae, V. Carruba, J. R. Masiero, R. C. Domingos, and M. Huaman. The Rafita asteroid family. MNRAS, 467(1):1016–1023, May 2017. doi: 10.1093/mnras/stx184.
2. C. Avdellidou, M. Delbo’, and A. Fienga. Exogenous origin of hydration on asteroid (16) Psyche: the role of hydrated asteroid families. MNRAS, 475(3):3419–3428, April 2018.
doi: 10.1093/mnras/sty017.
3. M. A. Barucci, M. Fulchignoni, J. Ji, S. Marchin, and N. Thomas. The Flybys of Asteroids 2867 Steins, 21 Lutetia, and 4179 Toutatis, pages 433–450. 2015. doi: 10.2458/azu
uapress 9780816532131-ch023.
4. I. N. Belskaya, Yu. G. Shkuratov, Yu. S. Efimov, N. M. Shakhovskoy, R. Gil-Hutton, A. Cellino, E. S. Zubko, A. A. Ovcharenko, S. Yu. Bondarenko, V. G. Shevchenko,
S. Fornasier, and C. Barbieri. The F-type asteroids with small inversion angles of polarization. Icarus, 178(1):213–221, Nov 2005. doi: 10.1016/j.icarus.2005.04.015.
5. I. N. Belskaya, S. Fornasier, G. P. Tozzi, R. Gil-Hutton, A. Cellino, K. Antonyuk, Yu. N. Krugly, A. N. Dovgopol, and S. Faggi. Refining the asteroid taxonomy by polarimetric observations. Icarus, 284:30–42, March 2017. doi: 10.1016/j.icarus.2016.11.003.
6. Irina N. Belskaya, Anny-Chantal Levasseur-Regourd, Alberto Cellino, Yuriy S. Efimov, Nikolay M. Shakhovskoy, Edith Hadamcik, and Philippe Bendjoya. Polarimetry of main belt asteroids: Wavelength dependence. Icarus, 199(1):97–105, January 2009. doi: 10.1016/j.icarus.2008.09.010.
7. R. Bianchi, F. Capaccioni, P. Cerroni, M. Coradini, E. Flamini, P. Hurren, G. Martelli,
and P. N. Smith. Experimental simulation of asteroidal fragmentation by macroscopic
hypervelocity impacts against free falling bodies. A&A, 139(1):1–6, October 1984.
8. Richard P. Binzel, Schelte J. Bus, Shui Xu, Jessica Sunshine, Thomas H. Burbine, A. William Neely, and Robert W. Brown. Rotationally resolved spectra of asteroid 16 Psyche. Icarus, 117(2):443–445, October 1995. doi: 10.1006/icar.1995.1170.
9. G. Borisov, M. Devog`ele, A. Cellino, S. Bagnulo, A. Christou, Ph Bendjoya, J. P. Rivet, L. Abe, D. Vernet, Z. Donchev, Yu Krugly, I. Belskaya, T. Bonev, D. Steeghs, D. Galloway, V. Dhillon, P. O’Brien, D. Pollacco, S. Poshyachinda, G. Ramsay, E. Thrane, K. Ackley, E. Rol, K. Ulaczyk, R. Cutter, and M. Dyer. Rotational variation of the linear polarization of the asteroid (3200) Phaethon as evidence for inhomogeneity in its surface properties. MNRAS, 480(1):L131–L135, October 2018. doi: 10.1093/mnrasl/sly140.
10. Jr. Bottke, William F. and H. Jay Melosh. Binary Asteroids and the Formation of Doublet Craters. Icarus, 124(2):372–391, December 1996. doi: 10.1006/icar.1996.0215.
11. Jr. Bottke, William F., David Vokrouhlick´y, David P. Rubincam, and David Nesvorn´y. The Yarkovsky and Yorp Effects: Implications for Asteroid Dynamics. Annual Review of Earth and Planetary Sciences, 34:157–191, May 2006. doi: 10.1146/annurev.earth. 34.031405.125154.
12. W. F. Bottke, D. Vokrouhlick´y, R. L. Ballouz, O. S. Barnouin, Jr. Connolly, H. C., C. Elder, S. Marchi, T. J. McCoy, P. Michel, M. C. Nolan, B. Rizk, D. J. Scheeres,
S. R. Schwartz, K. J. Walsh, and D. S. Lauretta. Interpreting the Cratering Histories of Bennu, Ryugu, and Other Spacecraft-explored Asteroids. AJ, 160(1):14, July 2020. doi: 10.3847/1538-3881/ab88d3.
13. E. Bowell and K. Lumme. Colorimetry and magnitudes of asteroids. In Tom Gehrels and Mildred Shapley Matthews, editors, Asteroids, pages 132–169. 1979.
14. Edward Bowell, Bruce Hapke, Deborah Domingue, Kari Lumme, Jouni Peltoniemi, and Alan W. Harris. Application of photometric models to asteroids. In Richard P. Binzel, Tom Gehrels, and Mildred Shapley Matthews, editors, Asteroids II, pages 524–556, January 1989.
15. P. Broglia and A. Manara. A search for rotational variations in the optical polarization of 3 Juno and 7 IRIS. A&A, 237(1):256–258, October 1990.
16. P. Broglia and A. Manara. A study of the polarimetric lightcurve of the asteroid 16 Psyche. A&A, 257(2):770–772, April 1992.
17. Schelte J. Bus and Richard P. Binzel. Phase II of the Small Main-Belt Asteroid Spectroscopic Survey. A Feature-Based Taxonomy. Icarus, 158(1):146–177, Jul 2002. doi: 10.1006/icar.2002.6856.
18. F. Capaccioni, P. Cerroni, M. Coradini, M. Di Martino, P. Farinella, E. Flamini, G. Martelli, P. Paolicchi, P. N. Smith, A. Woodward, and V. Zappala. Asteroidal catastrophic collisions simulated by hypervelocity impact experiments. Icarus, 66(3): 487–514, June 1986. doi: 10.1016/0019-1035(86)90087-4.
19. Albino Carbognani. The spin-barrier ratio for S and C-type main asteroids belt. Planet. Space Sci., 147:1–5, November 2017. doi: 10.1016/j.pss.2017.07.019.
20. B. Carry. Density of asteroids. Planet. Space Sci., 73(1):98–118, December 2012. doi: 10.1016/j.pss.2012.03.009.
21. J. H. Castro-Chac´on, R. Gil-Hutton, J. Ram´ırez V´elez, and M. Reyes-Ruiz. Polarimetric rotational curve of M-type asteroid (16) Psyche. Planet. Space Sci., 213:105428, April
2022. doi: 10.1016/j.pss.2022.105428.
21. V. Catullo, V. Zappala, P. Farinella, and P. Paolicchi. Analysis of the shape distribution of asteroids. A&A, 138(2):464–468, September 1984.
22. A. Cellino, R. Gil Hutton, E. F. Tedesco, M. Di Martino, and A. Brunini. Polarimetric Observations of Small Asteroids: Preliminary Results. Icarus, 138(1):129–140, Mar 1999. doi: 10.1006/icar.1998.6062.
23. A. Cellino, S. J. Bus, A. Doressoundiram, and D. Lazzaro. Spectroscopic Properties of Asteroid Families. In Asteroids III, pages 633–643. 2002.
24. A. Cellino, R. Gil Hutton, M. Di Martino, Ph. Bendjoya, I. N. Belskaya, and E. F. Tedesco. Asteroid polarimetric observations using the Torino UBVRI photopolarimeter. Icarus, 179(2):304–324, December 2005a. doi: 10.1016/j.icarus.2005.07.016.
25. A. Cellino, I. N. Belskaya, Ph. Bendjoya, M. Di Martino, R. Gil-Hutton, K. Muinonen, and E. F. Tedesco. The strange polarimetric behavior of Asteroid (234) Barbara. Icarus, 180(2):565–567, February 2006. doi: 10.1016/j.icarus.2005.09.001.
26. A. Cellino, S. Bagnulo, R. Gil-Hutton, P. Tanga, M. Ca˜nada-Assandri, and E. F. Tedesco. On the calibration of the relation between geometric albedo and polarimetric properties for the asteroids. MNRAS, 451(4):3473–3488, Aug 2015a. doi: 10.1093/mnras/stv1188.
27. A. Cellino, R. Gil-Hutton, and I. N. Belskaya. Asteroids. In Polarimetry of Stars and Planetary Systems, pages 360–378. 2015b.
28. A. Cellino, E. Ammannito, G. Magni, R. Gil-Hutton, E. F. Tedesco, I. N. Belskaya, M. C. De Sanctis, S. Schr¨oder, F. Preusker, and A. Manara. The Dawn exploration of (4) Vesta as the ‘ground truth’ to interpret asteroid polarimetry. MNRAS, 456(1):248–262, February 2016. doi: 10.1093/mnras/stv2683.
29. A. Cellino, S. Bagnulo, I. N. Belskaya, and A. A. Christou. Unusual polarimetric properties of (101955) Bennu: similarities with F-class asteroids and cometary bodies. MNRAS, 481(1):L49–L53, Nov 2018. doi: 10.1093/mnrasl/sly156.
30. A. Cellino, S. Bagnulo, P. Tanga, M. Devog`ele, Ph Bendjoya, E. Reilly, J. P. Rivet, and F. Spoto. Brang¨ane: a new family of Barbarian asteroids. MNRAS, 485(1):570–576, May 2019. doi: 10.1093/mnras/stz451.
31. Alberto Cellino, Fumi Yoshida, E. Anderlucci, Philippe Bendjoya, Mario Di Martino, Masateru Ishiguro, Akiko M. Nakamura, and Jun Saito. A polarimetric study of Asteroid 25143 Itokawa. Icarus, 179(2):297–303, December 2005b. doi: 10.1016/j.icarus. 2005.08.005.
32. John E. Chambers. Planetary accretion in the inner Solar System. Earth and Planetary Science Letters, 223(3-4):241–252, July 2004. doi: 10.1016/j.epsl.2004.04.031.
33. Chan-Kao Chang, Wing-Huen Ip, Hsing-Wen Lin, Yu-Chi Cheng, Chow-Choong Ngeow, Ting-Chang Yang, Adam Waszczak, Shrinivas R. Kulkarni, David Levitan, Branimir Sesar, Russ Laher, Jason Surace, and Thomas. A. Prince. 313 New Asteroid Rotation Periods from Palomar Transient Factory Observations. ApJ, 788(1):17, June 2014. doi: 10.1088/0004-637X/788/1/17.
34. Chan-Kao Chang, Wing-Huen Ip, Hsing-Wen Lin, Yu-Chi Cheng, Chow-Choong Ngeow, Ting-Chang Yang, Adam Waszczak, Shrinivas R. Kulkarni, David Levitan, Branimir Sesar, Russ Laher, Jason Surace, and Thomas. A. Prince. Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory. ApJS, 219(2):27, August 2015. doi: 10.1088/0067-0049/219/2/27.
35. Chan-Kao Chang, Hsing-Wen Lin, Wing-Huen Ip, Thomas A. Prince, Shrinivas R. Kulkarni, David Levitan, Russ Laher, and Jason Surace. Large Super-fast Rotator Hunting Using the Intermediate Palomar Transient Factory. ApJS, 227(2):20, December 2016. doi: 10.3847/0067-0049/227/2/20.
36. C. R. Chapman, D. Morrison, and B. Zellner. Surface Properties of Asteroids: A Synthesis of Polarimetry, Radiometry, and Spectrophotometry. Icarus, 25(1):104–130, May 1975. doi: 10.1016/0019-1035(75)90191-8.
37. W. P. Chen and S. C. L. Hu. Detection of a Proto-planetary Clump in the Habitable Zone of GM Cephei. In Nader Haghighipour, editor, Formation, Detection, and Characterization of Extrasolar Habitable Planets, volume 293, pages 74–76, April 2014. doi: 10.1017/S174392131301257X.
38. B. E. Clark, S. J. Bus, A. S. Rivkin, M. K. Shepard, and S. Shah. Spectroscopy of X-Type Asteroids. AJ, 128(6):3070–3081, December 2004. doi: 10.1086/424856.
39. G. J. Consolmagno, D. T. Britt, and R. J. Macke. The Density and Porosity of Carbonaceous Chondrites: A New Look. Meteoritics and Planetary Science Supplement, 43: 5038, August 2008.
40. D. R. Davis, C. R. Chapman, R. Greenberg, and S. J.Weidenschilling. Hirayama Families: Chips Off the Old Block or Collections of Rubble Piles? In Bulletin of the American Astronomical Society, volume 14, page 720, June 1982.
41. G. C. de El´ıa and A. Brunini. Collisional and dynamical evolution of the main belt and NEA population. A&A, 466(3):1159–1177, May 2007. doi: 10.1051/0004-6361: 20066046.
42. M. N. De Pr´a, N. Pinilla-Alonso, J. Carvano, J. Licandro, D. Morate, V. Lorenzi, J. de Le´on, H. Campins, and T. Moth´e-Diniz. A comparative analysis of the outer-belt primitive families. A&A, 643:A102, November 2020. doi: 10.1051/0004-6361/202038536.
43. F. DeMeo, R. P. Binzel, S. M. Slivan, and S. J. Bus. Bus-DeMeo Asteroid Taxonomy V1.0. NASA Planetary Data System, art. EAR-A-VARGBDET-5-BUSDEMEOTAXV1.0, July 2009.
44. F. E. DeMeo, C. M. O’D. Alexander, K. J. Walsh, C. R. Chapman, and R. P. Binzel. The Compositional Structure of the Asteroid Belt. In Asteroids IV, pages 13–41. 2015. doi: 10.2458/azu uapress 9780816532131-ch002.
45. M. Devog`ele, A. Cellino, S. Bagnulo, J. P. Rivet, P. Bendjoya, L. Abe, C. Pernechele, G. Massone, D. Vernet, P. Tanga, and C. Dimur. The Calern Asteroid Polarimetric Survey using the Torino polarimeter: assessment of instrument performances and first scientific results. MNRAS, 465(4):4335–4347, Mar 2017. doi: 10.1093/mnras/stw2952.
46. M. Devog`ele, A. Cellino, G. Borisov, Ph Bendjoya, J. P. Rivet, L. Abe, S. Bagnulo, A. Christou, D. Vernet, Z. Donchev, I. Belskaya, T. Bonev, and Yu N. Krugly. The phase-polarization curve of asteroid (3200) Phaethon. MNRAS, 479(3):3498–3508, Sep 2018a. doi: 10.1093/mnras/sty1587.
47. M. Devog`ele, P. Tanga, A. Cellino, Ph. Bendjoya, J. P. Rivet, J. Surdej, D. Vernet, J. M. Sunshine, S. J. Bus, L. Abe, S. Bagnulo, G. Borisov, H. Campins, B. Carry, J. Licandro, W. McLean, and N. Pinilla-Alonso. New polarimetric and spectroscopic evidence of anomalous enrichment in spinel-bearing calcium-aluminium-rich inclusions among L-type asteroids. Icarus, 304:31–57, April 2018b. doi: 10.1016/j.icarus.2017.12.026.
48. A. Dollfus and B. Zellner. Optical polarimetry of asteroids and laboratory samples. In Tom Gehrels and Mildred Shapley Matthews, editors, Asteroids, pages 170–183. 1979.
49. A. Dollfus, M.Wolff, J. E. Geake, D. F. Lupishko, and L. M. Dougherty. Photopolarimetry of asteroids. In Richard P. Binzel, Tom Gehrels, and Mildred Shapley Matthews, editors, Asteroids II, pages 594–616, January 1989.
50. Daniel D. Durda, William F. Bottke, David Nesvorn´y, Brian L. Enke, William J. Merline, Erik Asphaug, and Derek C. Richardson. Size-frequency distributions of fragments from SPH/ N-body simulations of asteroid impacts: Comparison with observed asteroid families. Icarus, 186(2):498–516, February 2007. doi: 10.1016/j.icarus.2006.09.013.
51. Daniel D. Durda, Adriano Campo Bagatin, Rafael A. Alema˜n, George J. Flynn, Melissa M. Strait, Angela N. Clayton, and Emma B. Patmore. The shapes of fragments from catastrophic disruption events: Effects of target shape and impact speed. Planet. Space Sci., 107:77–83, March 2015. doi: 10.1016/j.pss.2014.10.006.
52. J. Durech, V. Sidorin, and M. Kaasalainen. DAMIT: a database of asteroid models. A&A, 513:A46, April 2010. doi: 10.1051/0004-6361/200912693.
53. L. T. Elkins-Tanton, E. Asphaug, J. F. Bell III, H. Bercovici, B. Bills, R. Binzel, W. F. Bottke, S. Dibb, D. J. Lawrence, S. Marchi, T. J. McCoy, R. Oran, R. S. Park, P. N. Peplowski, C. A. Polanskey, T. H. Prettyman, C. T. Russell, L. Schaefer, B. P. Weiss, M. A. Wieczorek, D. A. Williams, and M. T. Zuber. Observations, meteorites, and models: A preflight assessment of the composition and formation of (16) psyche. Journal of Geophysical Research: Planets, 125(3):e2019JE006296, 2020. doi: 10.1029/2019JE006296. URL https://agupubs.onlinelibrary.wiley. com/doi/abs/10.1029/2019JE006296. e2019JE006296 2019JE006296.
54. P. Farinella, P. Paolicchi, and V. Zappala. The asteroids as outcomes of catastrophic collisions. Icarus, 52(3):409–433, December 1982. doi: 10.1016/0019-1035(82)90003-3.
55. S. Fornasier, I. N. Belskaya, Yu. G. Shkuratov, C. Pernechele, C. Barbieri, E. Giro, and H. Navasardyan. Polarimetric survey of asteroids with the Asiago telescope. A&A, 455 (1):371–377, August 2006. doi: 10.1051/0004-6361:20064836.
56. K. Fox, I. P. Williams, and D. W. Hughes. The ’Geminid’ asteroid (1983 TB) and its orbital evolution. MNRAS, 208:11P–15P, June 1984. doi: 10.1093/mnras/208.1.11P.
57. A. Fujiwara, G. Kamimoto, and A. Tsukamoto. Destruction of basaltic bodies by highvelocity impact. Icarus, 31(2):277–288, June 1977. doi: 10.1016/0019-1035(77)90038-0.
58. A. Fujiwara, G. Kamimoto, and A. Tsukamoto. Expected shape distribution of asteroids obtained from laboratory impact experiments. Nature, 272:602, April 1978. doi: 10. 1038/272602a0.
59. A. Fujiwara, P. Cerroni, D. R. Davis, E. Ryan, M. di Martino, K. Holsapple, and K. Housen. Experiments and scaling laws for catastrophic collisions. In Richard P. Binzel, Tom Gehrels, and Mildred Shapley Matthews, editors, Asteroids II, pages 240– 265, January 1989.
60. A. Fujiwara, J. Kawaguchi, D. K. Yeomans, M. Abe, T. Mukai, T. Okada, J. Saito, H. Yano, M. Yoshikawa, D. J. Scheeres, O. Barnouin-Jha, A. F. Cheng, H. Demura, R. W. Gaskell, N. Hirata, H. Ikeda, T. Kominato, H. Miyamoto, A. M. Nakamura, R. Nakamura, S. Sasaki, and K. Uesugi. The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa. Science, 312(5778):1330–1334, June 2006. doi: 10.1126/science.1125841.
61. J. E. Geake and A. Dollfus. Planetary surface texture and albedo from parameter plots of optical polarization data. MNRAS, 218:75–91, January 1986. doi: 10.1093/mnras/218.1.75.
62. R. Gil-Hutton. Polarimetry of M-type asteroids. A&A, 464(3):1127–1132, Mar 2007. doi: 10.1051/0004-6361:20066348.
63. R. Gil-Hutton and M. Ca˜nada-Assandri. Polarimetric survey of main-belt asteroids. I. Results for fifty seven S-, L-, and K-type objects. A&A, 529:A86, May 2011. doi: 10.1051/0004-6361/201015402.
64. R. Gil-Hutton and M. Ca˜nada-Assandri. Polarimetric survey of main-belt asteroids. II. Results for 58 B- and C-type objects. A&A, 539:A115, Mar 2012. doi: 10.1051/0004-6361/201117237.
65. Philippe Gillet and Ahmed El Goresy. Shock Events in the Solar System: The Message from Minerals in Terrestrial Planets and Asteroids. Annual Review of Earth and Planetary Sciences, 41:257–285, May 2013. doi: 10.1146/annurev-earth-042711-105538.
66. J. Gradie and E. Tedesco. Compositional Structure of the Asteroid Belt. Science, 216 (4553):1405–1407, June 1982. doi: 10.1126/science.216.4553.1405.
67. S. F. Green, A. J. Meadows, and J. K. Davies. Infrared observations of the extinct cometary candidate minor planet (3200) 1983TB. MNRAS, 214:29P–36P, June 1985. doi: 10.1093/mnras/214.1.29P.
68. B. A. S. Gustafson. Geminid meteoroids traced to cometary activity on Phaethon. A&A, 225(2):533–540, November 1989.
69. J. Hanuˇs, M. Viikinkoski, F. Marchis, J. ˇ Durech, M. Kaasalainen, M. Delbo’, D. Herald, E. Frappa, T. Hayamizu, S. Kerr, S. Preston, B. Timerson, D. Dunham, and J. Talbot. Volumes and bulk densities of forty asteroids from ADAM shape modeling. A&A, 601: A114, May 2017. doi: 10.1051/0004-6361/201629956.
70. A. W. Harris. The Rotation Rates of Very Small Asteroids: Evidence for ’Rubble Pile’ Structure. In Lunar and Planetary Science Conference, volume 27 of Lunar and Planetary Science Conference, page 493, March 1996.
71. Alan W. Harris, Eugene G. Fahnestock, and Petr Pravec. On the shapes and spins of “rubble pile” asteroids. Icarus, 199(2):310–318, February 2009. doi: 10.1016/j.icarus. 2008.09.012.
72. Tom´aˇs Henych and Petr Pravec. Slowly increasing elongations of non-spherical asteroids caused by collisions. MNRAS, 454(2):1704–1710, December 2015. doi: 10.1093/mnras/stv2133.
73. Carl W. Hergenrother and Robert J. Whiteley. A survey of small fast rotating asteroids among the near-Earth asteroid population. Icarus, 214(1):194–209, July 2011. doi: 10.1016/j.icarus.2011.03.023.
74. Masatoshi Hirabayashi, Daniel J. Scheeres, Diego Paul S´anchez, and Travis Gabriel. Constraints on the Physical Properties of Main Belt Comet P/2013 R3 from its Breakup Event. ApJ, 789(1):L12, July 2014. doi: 10.1088/2041-8205/789/1/L12.
75. Keith A. Holsapple. Spin limits of Solar System bodies: From the small fast-rotators to 2003 EL61. Icarus, 187(2):500–509, April 2007. doi: 10.1016/j.icarus.2006.08.012.
76. Kevin R. Housen, Keith A. Holsapple, and Michael E. Voss. Compaction as the origin of the unusual craters on the asteroid Mathilde. Nature, 402(6758):155–157, November 1999. doi: 10.1038/45985.
77. P. C. Huang, W. P. Chen, M. Mugrauer, R. Bischoff, J. Budaj, O. Burkhonov, S. Ehgamberdiev, R. Errmann, Z. Garai, H. Y. Hsiao, C. L. Hu, R. Janulis, E. L. N. Jensen, S. Kiyota, K. Kuramoto, C. S. Lin, H. C. Lin, J. Z. Liu, O. Lux, H. Naito, R. Neuh¨auser, J. Ohlert, E. Pakˇstien˙e, T. Pribulla, J. K. T. Qvam, St. Raetz, S. Sato, M. Schwartz, E. Semkov, S. Takagi, D.Wagner, M.Watanabe, and Yu Zhang. Diagnosing the Clumpy
Protoplanetary Disk of the UXor Type Young Star GM Cephei. ApJ, 871(2):183, Feb 2019. doi: 10.3847/1538-4357/aaf793.
78. W. H. Ip. On three types of fragmentation processes observed in the asteroid belt. Icarus, 40(3):418–422, December 1979. doi: 10.1016/0019-1035(79)90034-4.
79. Takashi Ito, Masateru Ishiguro, Tomoko Arai, Masataka Imai, Tomohiko Sekiguchi, Yoonsoo P. Bach, Yuna G. Kwon, Masanori Kobayashi, Ryo Ishimaru, Hiroyuki Naito, Makoto Watanabe, and Kiyoshi Kuramoto. Extremely strong polarization of an active asteroid (3200) Phaethon. Nature Communications, 9:2486, June 2018. doi: 10.1038/s41467-018-04727-2.
80. M. Kaasalainen, J. Torppa, and K. Muinonen. Optimization Methods for Asteroid Lightcurve Inversion. II. The Complete Inverse Problem. Icarus, 153(1):37–51, Sep 2001. doi: 10.1006/icar.2001.6674.
81. D. G. Korycansky and Erik Asphaug. Impact evolution of asteroid shapes. 1. random mass redistribution. Icarus, 163(2):374–388, June 2003. doi: 10.1016/S0019-1035(03)00079-4.
82. D. S. Lauretta, D. N. Dellagiustina, C. A. Bennett, D. R. Golish, K. J. Becker, S. S. Balram-Knutson, O. S. Barnouin, T. L. Becker, W. F. Bottke, W. V. Boynton, H. Campins, B. E. Clark, H. C. Connolly, C. Y. Drouet D’Aubigny, J. P. Dworkin, J. P. Emery, H. L. Enos, V. E. Hamilton, C. W. Hergenrother, E. S. Howell, M. R. M. Izawa, H. H. Kaplan, M. C. Nolan, B. Rizk, H. L. Roper, D. J. Scheeres, P. H. Smith, K. J. Walsh, C. W. V. Wolner, and Osiris-Rex Team. The unexpected surface of asteroid (101955) Bennu. Nature, 568(7750):55–60, March 2019. doi: 10.1038/s41586-019-1033-6.
83. D. Lazzaro, C. A. Angeli, J. M. Carvano, T. Moth´e-Diniz, R. Duffard, and M. Florczak. S 3OS 2: the visible spectroscopic survey of 820 asteroids. Icarus, 172(1):179–220, Nov 2004. doi: 10.1016/j.icarus.2004.06.006.
84. J. Y. Li, P. Helfenstein, B. Buratti, D. Takir, and B. E. Clark. Asteroid Photometry. In Asteroids IV, pages 129–150. 2015. doi: 10.2458/azu uapress 9780816532131-ch007.
85. Chien-Hsien Lin, Wing-Huen Ip, Zhong-Yi Lin, Yu-Chi Cheng, Hsing-Wen Lin, and Chan-Kao Chang. Photometric survey and taxonomic identifications of 92 near-Earth asteroids. Planet. Space Sci., 152:116–135, March 2018. doi: 10.1016/j.pss.2017.12.019.
86. A. Mainzer, J. Bauer, R. M. Cutri, T. Grav, J. Masiero, R. Beck, P. Clarkson, T. Conrow, J. Dailey, P. Eisenhardt, B. Fabinsky, S. Fajardo-Acosta, J. Fowler, C. Gelino, C. Grillmair, I. Heinrichsen, M. Kendall, J. Davy Kirkpatrick, F. Liu, F. Masci, H. McCallon, C. R. Nugent, M. Papin, E. Rice, D. Royer, T. Ryan, P. Sevilla, S. Sonnett, R. Stevenson,
D. B. Thompson, S. Wheelock, D. Wiemer, M. Wittman, E. Wright, and L. Yan.
Initial Performance of the NEOWISE Reactivation Mission. ApJ, 792(1):30, September 2014. doi: 10.1088/0004-637X/792/1/30.
87. A. Marciniak, P. Bartczak, T. Santana-Ros, T. Micha lowski, P. Antonini, R. Behrend, C. Bembrick, L. Bernasconi, W. Borczyk, F. Colas, J. Coloma, R. Crippa, N. Esseiva, M. Fagas, M. Fauvaud, S. Fauvaud, D. D. M. Ferreira, R. P. Hein Bertelsen, D. Higgins, R. Hirsch, J. J. E. Kajava, K. Kami´nski, A. Kryszczy´nska, T. Kwiatkowski, F. Manzini, J. Micha lowski, M. J. Micha lowski, A. Paschke, M. Poli´nska, R. Poncy, R. Roy, G. Santacana, K. Sobkowiak, M. Stasik, S. Starczewski, F. Velichko, H.Wucher,
and T. Zafar. Photometry and models of selected main belt asteroids. IX. Introducing interactive service for asteroid models (ISAM). A&A, 545:A131, September 2012. doi: 10.1051/0004-6361/201219542.
88. J. R. Masiero, F. E. DeMeo, T. Kasuga, and A. H. Parker. Asteroid Family Physical Properties, pages 323–340. 2015. doi: 10.2458/azu uapress 9780816532131-ch017.
89. Joseph Masiero. Albedo heterogeneity on the surface of (1943) Anteros. Icarus, 207(2): 795–799, June 2010. doi: 10.1016/j.icarus.2009.12.033.
90. Joseph Masiero, Robert Jedicke, Josef ˇ Durech, Stephen Gwyn, Larry Denneau, and Jeff Larsen. The Thousand Asteroid Light Curve Survey. Icarus, 204(1):145–171, November 2009. doi: 10.1016/j.icarus.2009.06.012.
91. Joseph R. Masiero, A. K. Mainzer, T. Grav, J. M. Bauer, E. L. Wright, R. S. McMillan, D. J. Tholen, and A. W. Blain. A Revised Asteroid Polarization-Albedo Relationship Using WISE/NEOWISE Data. ApJ, 749(2):104, April 2012. doi: 10.1088/0004-637X/749/2/104.
92. Joseph R. Masiero, A. K. Mainzer, J. M. Bauer, T. Grav, C. R. Nugent, and R. Stevenson. Asteroid Family Identification Using the Hierarchical Clustering Method and WISE/-NEOWISE Physical Properties. ApJ, 770(1):7, June 2013. doi: 10.1088/0004-637X/770/1/7.
93. Alexis Matter, Marco Delbo, Benoit Carry, and Sebastiano Ligori. Evidence of a metalrich surface for the Asteroid (16) Psyche from interferometric observations in the thermal infrared. Icarus, 226(1):419–427, September 2013. doi: 10.1016/j.icarus.2013.06.004.
94. T. B. McCord, J. Y. Li, J. P. Combe, H. Y. McSween, R. Jaumann, V. Reddy, F. Tosi, D. A. Williams, D. T. Blewett, D. Turrini, E. Palomba, C. M. Pieters, M. C. de Sanctis, E. Ammannito, M. T. Capria, L. Le Corre, A. Longobardo, A. Nathues, D. W. Mittlefehldt, S. E. Schr¨oder, H. Hiesinger, A. W. Beck, F. Capaccioni, U. Carsenty, H. U. Keller, B. W. Denevi, J. M. Sunshine, C. A. Raymond, and C. T. Russell. Dark material on Vesta from the infall of carbonaceous volatile-rich material. Nature, 491 (7422):83–86, November 2012. doi: 10.1038/nature11561.
95. P. Michel, F. E. DeMeo, and W. F. Bottke. Asteroids: Recent Advances and
New Perspectives. In Asteroids IV, pages 3–10. 2015. doi: 10.2458/azu uapress9780816532131-ch001.
96. Patrick Michel, Willy Benz, and Derek C. Richardson. Disruption of fragmented parent bodies as the origin of asteroid families. Nature, 421(6923):608–611, February 2003. doi: 10.1038/nature01364.
97. Tatsuhiro Michikami, Akiko M. Nakamura, and Naru Hirata. The shape distribution of boulders on Asteroid 25143 Itokawa: Comparison with fragments from impact experiments. Icarus, 207(1):277–284, May 2010. doi: 10.1016/j.icarus.2009.10.008.
98. Tatsuhiro Michikami, Axel Hagermann, Tokiyuki Kadokawa, Akifumi Yoshida, Akira Shimada, Sunao Hasegawa, and Akira Tsuchiyama. Fragment shapes in impact experiments ranging from cratering to catastrophic disruption. Icarus, 264:316–330, January 2016. doi: 10.1016/j.icarus.2015.09.038.
99. F. Migliorini, V. Zappal`a, R. Vio, and A. Cellino. Interlopers within asteroid families.Icarus, 118(2):271–291, December 1995. doi: 10.1006/icar.1995.1191.
100. Andrea Milani, Alberto Cellino, Zoran Kneˇzevi´c, Bojan Novakovi´c, Federica Spoto, and Paolo Paolicchi. Asteroid families classification: Exploiting very large datasets. Icarus, 239:46–73, September 2014. doi: 10.1016/j.icarus.2014.05.039.
101. M. I. Mishchenko, V. K. Rosenbush, N. N. Kiselev, D. F. Lupishko, V. P. Tishkovets, V. G. Kaydash, I. N. Belskaya, Y. S. Efimov, and N. M. Shakhovskoy. Methodology of polarimetric observations, pages 117–122. 2010.
102. Thierry Montmerle, Jean-Charles Augereau, Marc Chaussidon, Mathieu Gounelle, Bernard Marty, and Alessandro Morbidelli. From Suns to Life: A Chronological Approach to the History of Life on Earth 3. Solar System Formation and Early Evolution: the First 100 Million Years. Earth Moon and Planets, 98(1-4):39–95, June 2006. doi: 10.1007/s11038-006-9087-5.
103. A. Morbidelli, J. I. Lunine, D. P. O’Brien, S. N. Raymond, and K. J. Walsh. Building Terrestrial Planets. Annual Review of Earth and Planetary Sciences, 40(1):251–275, May 2012. doi: 10.1146/annurev-earth-042711-105319.
104. K. Muinonen, J. Piironen, Yu. G. Shkuratov, A. Ovcharenko, and B. E. Clark. Asteroid Photometric and Polarimetric Phase Effects. In Asteroids III, pages 123–138. 2002.
105. K. Muinonen, A. Penttil¨a, A. Cellino, I. N. Belskaya, M. Delb`o, A. C. Levasseur-Regourd, and E. F. Tedesco. Asteroid photometric and polarimetric phase curves: Joint linearexponential modeling. Meteoritics and Planetary Science, 44(12):1937–1946, Jan 2009. doi: 10.1111/j.1945-5100.2009.tb02003.x.
106. Hiroyuki Nakayama, Yasumasa Fujii, Masateru Ishiguro, Ryosuke Nakamura, Sozo Yokogawa, Fumi Yoshida, and Tadashi Mukai. Observations of Polarization and Brightness Variations with the Rotation for Asteroids 9 Metis, 52 Europa, and 1036 Ganymed. Icarus, 146(1):220–231, July 2000. doi: 10.1006/icar.2000.6396.
107. D. Nesvorny. Nesvorny HCM Asteroid Families V3.0. NASA Planetary Data System, art. EAR-A-VARGBDET-5-NESVORNYFAM-V3.0, December 2015.
108. David Nesvorn´y, William F. Bottke, David Vokrouhlick´y, Alessandro Morbidelli, and Robert Jedicke. Asteroid families. In Daniela Lazzaro, Sylvio Ferraz-Mello, and Julio Angel Fern´andez, editors, Asteroids, Comets, Meteors, volume 229, pages 289–299, January 2006. doi: 10.1017/S1743921305006800.
109. C. R. Nugent, A. Mainzer, J. Masiero, J. Bauer, R. M. Cutri, T. Grav, E. Kramer, S. Sonnett, R. Stevenson, and E. L. Wright. NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos. ApJ, 814(2):117, December 2015. doi: 10.1088/0004-637X/814/2/117.
110. Steven. J. Ostro, Jean-Luc Margot, Lance A. M. Benner, Jon D. Giorgini, Daniel J. Scheeres, Eugene G. Fahnestock, Stephen B. Broschart, Julie Bellerose, Michael C. Nolan, Christopher Magri, Petr Pravec, Petr Scheirich, Randy Rose, Raymond F. Jurgens, Eric M. De Jong, and Shigeru Suzuki. Radar Imaging of Binary Near-Earth Asteroid (66391) 1999 KW4. Science, 314(5803):1276–1280, November 2006. doi:10.1126/science.1133622.
111. Kang-Shian Pan and Wing-Huen Ip. Polarimetric observations of asteroids of different taxonomic classes from Lulin Observatory in Taiwan. Planet. Space Sci., 212:105412, March 2022. doi: 10.1016/j.pss.2021.105412.
112. D. Polishook and N. Brosch. Photometry and spin rate distribution of small-sized main belt asteroids. Icarus, 199(2):319–332, February 2009. doi: 10.1016/j.icarus.2008.10.020.
113. P. Pravec, A. W. Harris, and T. Michalowski. Asteroid Rotations. In Asteroids III, pages 113–122. 2002.
114. Petr Pravec and Alan W. Harris. Fast and Slow Rotation of Asteroids. Icarus, 148(1):12–20, November 2000. doi: 10.1006/icar.2000.6482.
115. W. Uwe Reimold and Fred Jourdan. IMPACT! – BOLIDES, CRATERS, AND CATASTROPHES. Elements, 8(1):19–24, 02 2012. ISSN 1811-5209. doi: 10.2113/gselements. 8.1.19. URL https://doi.org/10.2113/gselements.8.1.19.
116. A. S. Rivkin, E. S. Howell, L. A. Lebofsky, B. E. Clark, and D. T. Britt. The nature of M-class asteroids from 3-micron observations. Icarus, 145(2):351–368, June 2000. doi:10.1006/icar.2000.6354.
117. Juan A. Sanchez, Vishnu Reddy, Michael K. Shepard, Cristina Thomas, Edward A. Cloutis, Driss Takir, Albert Conrad, Cain Kiddell, and Daniel Applin. Detection of Rotational Spectral Variation on the M-type Asteroid (16) Psyche. AJ, 153(1):29, January 2017. doi: 10.3847/1538-3881/153/1/29.
118. P. S´anchez and D. J. Scheeres. The strength of regolith and rubble pile asteroids. , 49(5):788–811, May 2014. doi: 10.1111/maps.12293.
119. Shuji Sato, Po Chieh Huang, Wen Ping Chen, Takahiro Zenno, Chakali Eswaraiah, Bo He Su, Shinsuke Abe, Daisuke Kinoshita, and Jia Wei Wang. Triple Range Imager and POLarimeter (TRIPOL)—a compact and economical optical imaging polarimeter for small telescopes. Research in Astronomy and Astrophysics, 19(9):136, Sep 2019. doi:10.1088/1674-4527/19/9/136.
120. D. J. Scheeres, C. M. Hartzell, P. S´anchez, and M. Swift. Scaling forces to asteroid surfaces: The role of cohesion. Icarus, 210(2):968–984, December 2010. doi: 10.1016/j.icarus.2010.07.009.
121. Gary D. Schmidt, Richard Elston, and Olivia L. Lupie. The Hubble Space Telescope Northern-Hemisphere Grid of Stellar Polarimetric Standards. AJ, 104:1563, Oct 1992. doi: 10.1086/116341.
122. K. Serkowski. Polarimeters for Optical Astronomy. In T. Gehrels, editor, IAU Colloq. 23: Planets, Stars, and Nebulae: Studied with Photopolarimetry, page 135, January 1974.
123. N M Shakhovskoi and Yu S Efimov. Polarization observations of nonstable stars and extragalactic objects. I. Equipment, method of observation, and reduction. Izv. Krym. Astrofiz. Observ., 45:90–110, Jun 1972.
124. Michael K. Shepard, James Richardson, Patrick A. Taylor, Linda A. Rodriguez-Ford, Al Conrad, Imke de Pater, Mate Adamkovics, Katherine de Kleer, Jared R. Males, Katie M. Morzinski, Laird M. Close, Mikko Kaasalainen, Matti Viikinkoski, Bradley Timerson, Vishnu Reddy, Christopher Magri, Michael C. Nolan, Ellen S. Howell, Lance A. M. Benner, Jon D. Giorgini, Brian D. Warner, and Alan W. Harris. Radar observations and shape model of asteroid 16 Psyche. Icarus, 281:388–403, January 2017. doi:10.1016/j.icarus.2016.08.011.
125. K. Shinokawa, S. Takahashi, K. Ogawa, F. Yoshida, T. Minato, T. Mukai, and K. Kawabata. Observations of photopolarimetric variation with the rotation of asteroids, 3 Juno and 216 Kleopatra. Mem. Soc. Astron. Italiana, 73(3):658, September 2002.
126. J. Souchay, C. Lhotka, G. Heron, Y. Herv´e, V. Puente, and M. Folgueira Lopez. Changes of spin axis and rate of the asteroid (99942) Apophis during the 2029 close encounter with Earth: A constrained model. A&A, 617:A74, September 2018. doi: 10.1051/ 0004-6361/201832914.
127. Federica Spoto, Andrea Milani, and Zoran Kneˇzevi´c. Asteroid family ages. Icarus, 257:275–289, September 2015. doi: 10.1016/j.icarus.2015.04.041.
128. Robert G. Strom, Renu Malhotra, Takashi Ito, Fumi Yoshida, and David A. Kring. The Origin of Planetary Impactors in the Inner Solar System. Science, 309(5742):1847–1850, September 2005. doi: 10.1126/science.1113544.
129. Jessica Sunshine, L. Kolokolova, Jr. Connolly, H. C., T. J. McCoy, S. J. Bus, and J. R. Masiero. The Role of Mineralogy in Producing Unusual Polarization Effects in CAI-Rich Asteroids. In AAS/Division for Planetary Sciences Meeting Abstracts #40, volume 40 of AAS/Division for Planetary Sciences Meeting Abstracts, page 60.07, September 2008.
130. Gyula M. Szab´o and L´aszl´o L. Kiss. The shape distribution of asteroid families: Evidence for evolution driven by small impacts. Icarus, 196(1):135–143, July 2008. doi: 10.1016/j.icarus.2008.01.019.
131. S. Takahashi, F. Yoshida, K. Shinokawa, T. Mukai, and K. S. Kawabata. Simultaneous Photometric and Polarimetric Observations of Asteroid 3 Juno. AJ, 138(3):951–955, September 2009. doi: 10.1088/0004-6256/138/3/951.
132. D. Takir, V. Reddy, J. A. Sanchez, M. K. Shepard, and J. P. Emery. Investigating the Source of Water and/or Hydroxyl on Asteroid (16) Psyche. In AGU Fall Meeting Abstracts, volume 2017, pages P33G–01, December 2017a.
133. Driss Takir, Vishnu Reddy, Juan A. Sanchez, Michael K. Shepard, and Joshua P. Emery. Detection of Water and/or Hydroxyl on Asteroid (16) Psyche. AJ, 153(1):31, January 2017b. doi: 10.3847/1538-3881/153/1/31.
134. P. Tanga, A. Cellino, P. Michel, V. Zappal`a, P. Paolicchi, and A. Dell’Oro. On the Size Distribution of Asteroid Families: The Role of Geometry. Icarus, 141(1):65–78, September 1999. doi: 10.1006/icar.1999.6148.
135. E. F. Tedesco, D. J. Tholen, and B. Zellner. The eight-color asteroid survey : standard stars. AJ, 87:1585–1592, November 1982. doi: 10.1086/113248.
136. Edward F. Tedesco, Paul V. Noah, Meg Noah, and Stephan D. Price. The Supplemental IRAS Minor Planet Survey. AJ, 123(2):1056–1085, February 2002. doi: 10.1086/338320.
137. D. J. Tholen. Asteroid taxonomic classifications. In Richard P. Binzel, Tom Gehrels, and Mildred Shapley Matthews, editors, Asteroids II, pages 1139–1150, Jan 1989.
138. David James Tholen. Asteroid Taxonomy from Cluster Analysis of Photometry. PhD thesis, University of Arizona, Tucson, Sep 1984.
139. D. Turrini, V. Svetsov, G. Consolmagno, S. Sirono, and S. Pirani. Olivine on Vesta as exogenous contaminants brought by impacts: Constraints from modeling Vesta’s collisional history and from impact simulations. Icarus, 280:328–339, December 2016. doi: 10.1016/j.icarus.2016.07.009.
140. J. Veverka. The Physical Meaning of Phase Coefficients. In T. Gehrels, editor, NASA Special Publication, volume 267, page 79. 1971.
141. Kevin J.Walsh, Derek C. Richardson, and Patrick Michel. Spin-up of rubble-pile asteroids: Disruption, satellite formation, and equilibrium shapes. Icarus, 220(2):514–529, August 2012. doi: 10.1016/j.icarus.2012.04.029.
142. Jia-Wei Wang, Shih-Ping Lai, Chakali Eswaraiah, Dan P. Clemens, Wen-Ping Chen, and Anil K. Pandey. Multiwavelength Stellar Polarimetry of the Filamentary Cloud IC5146. I. Dust Properties. ApJ, 849(2):157, Nov 2017. doi: 10.3847/1538-4357/aa937f.
143. J. F. C. Wardle and P. P. Kronberg. The linear polarization of quasi-stellar radio sources at 3.71 and 11.1 centimeters. ApJ, 194:249–255, Dec 1974. doi: 10.1086/153240.
144. Brian D. Warner, Alan W. Harris, and Petr Pravec. The asteroid lightcurve database. Icarus, 202(1):134–146, July 2009. doi: 10.1016/j.icarus.2009.02.003.
145. Adam Waszczak, Chan-Kao Chang, Eran O. Ofek, Russ Laher, Frank Masci, David Levitan, Jason Surace, Yu-Chi Cheng, Wing-Huen Ip, Daisuke Kinoshita, George Helou, Thomas A. Prince, and Shrinivas Kulkarni. Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry. AJ, 150(3):75, September 2015. doi: 10.1088/0004-6256/150/3/75.
146. S. Watanabe, M. Hirabayashi, N. Hirata, Na. Hirata, R. Noguchi, Y. Shimaki, H. Ikeda, E. Tatsumi, M. Yoshikawa, S. Kikuchi, H. Yabuta, T. Nakamura, S. Tachibana, Y. Ishihara, T. Morota, K. Kitazato, N. Sakatani, K. Matsumoto, K. Wada, H. Senshu, C. Honda, T. Michikami, H. Takeuchi, T. Kouyama, R. Honda, S. Kameda, T. Fuse, H. Miyamoto, G. Komatsu, S. Sugita, T. Okada, N. Namiki, M. Arakawa, M. Ishiguro, M. Abe, R. Gaskell, E. Palmer, O. S. Barnouin, P. Michel, A. S. French, J. W. McMahon, D. J. Scheeres, P. A. Abell, Y. Yamamoto, S. Tanaka, K. Shirai, M. Matsuoka, M. Yamada, Y. Yokota, H. Suzuki, K. Yoshioka, Y. Cho, S. Tanaka, N. Nishikawa, T. Sugiyama, H. Kikuchi, R. Hemmi, T. Yamaguchi, N. Ogawa, G. Ono, Y. Mimasu, K. Yoshikawa, T. Takahashi, Y. Takei, A. Fujii, C. Hirose, T. Iwata, M. Hayakawa, S. Hosoda, O. Mori, H. Sawada, T. Shimada, S. Soldini, H. Yano, R. Tsukizaki,
M. Ozaki, Y. Iijima, K. Ogawa, M. Fujimoto, T. M. Ho, A. Moussi, R. Jaumann,
J. P. Bibring, C. Krause, F. Terui, T. Saiki, S. Nakazawa, and Y. Tsuda. Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top-shaped rubble pile. Science, 364(6437):268–272, April 2019. doi: 10.1126/science.aav8032.
147. F. L. Whipple. 1983 TB and the Geminid Meteors. IAU Circ., 3881:1, October 1983.
148. S. L. Wilkison, T. J. McCoy, J. E. McCamant, M. S. Robinson, and D. T. Britt. Porosity and density of ordinary chondrites: Clues to the formation of friable and porous ordinary chondrites. Meteoritics and Planetary Science, 38(10):1533–1546, October 2003. doi:10.1111/j.1945-5100.2003.tb00256.x.
149. M. Wolff. Polarization of light reflected from rough planetary surface. Appl. Opt., 14(6):1395–1405, June 1975. doi: 10.1364/AO.14.001395.
150. Jijin Yang, Joseph I. Goldstein, and Edward R. D. Scott. Iron meteorite evidence for early formation and catastrophic disruption of protoplanets. Nature, 446(7138):888–891, April 2007. doi: 10.1038/nature05735.
151. V. Zappala and A. Cellino. Asteroid Families. In Andrea Milani, Michel di Martino, and A. Cellino, editors, Asteroids, Comets, Meteors 1993, volume 160, page 395, January 1994.
152. V. Zappal`a, A. Cellino, A. Dell’oro, F. Migliorini, and P. Paolicchi. Reconstructing the Original Ejection Velocity Fields of Asteroid Families. Icarus, 124(1):156–180, November 1996. doi: 10.1006/icar.1996.0196.
153. Vincenzo Zappala, Alberto Cellino, Paolo Farinella, and Zoran Knezevic. Asteroid Families. I. Identification by Hierarchical Clustering and Reliability Assessment. AJ, 100:2030, December 1990. doi: 10.1086/115658.
154. B. Zellner. Polarimetric Albedos of Asteroids. In Bulletin of the American Astronomical Society, volume 5, page 388, September 1973.
155. B. Zellner, T. Gehrels, and J. Gradie. Minor planets and related objects. XVI. Polarimetric diameters. AJ, 79:1100–1110, Oct 1974. doi: 10.1086/111660.
156. B. Zellner, D. J. Tholen, and E. F. Tedesco. The eight-color asteroid survey: Results for 589 minor planets. Icarus, 61(3):355–416, March 1985. doi: 10.1016/0019-1035(85) 90133-2.
157. Meng-Hua Zhu, Wenzhe Fa, Wing-Huen Ip, Jiangchuan Huang, Tiantian Liu, Linzhi Meng, Jun Yan, Aoao Xu, Zesheng Tang, Xiaolei Wang, and Dong Qiao. Morphology of asteroid (4179) Toutatis as imaged by Chang’E-2 spacecraft. Geophys. Res. Lett., 41(2):328–333, January 2014. doi: 10.1002/2013GL058914.
指導教授 葉永烜(Wing-Huen Ip) 審核日期 2022-9-1
推文 facebook   plurk   twitter   funp   google   live   udn   HD   myshare   reddit   netvibes   friend   youpush   delicious   baidu   
網路書籤 Google bookmarks   del.icio.us   hemidemi   myshare   

若有論文相關問題，請聯絡國立中央大學圖書館推廣服務組 TEL:(03)422-7151轉57407，或E-mail聯絡  - 隱私權政策聲明