Rotationally Resolved Spectroscopic Observations of Asteroids using Lulin One-meter Telescope

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：56

、訪客IP：3.133.118.164

姓名

戴志仰(Chih-Yang Tai) 查詢紙本館藏

畢業系所

天文研究所

論文名稱

(Rotationally Resolved Spectroscopic Observations of Asteroids using Lulin One-meter Telescope)

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]

本電子論文使用權限為同意立即開放。
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。
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)

小行星是太陽系中數量最多的成員。小行星的表面成分對決定他們的演化歷史以及和太陽系其他天體的互動來說是重要的因素。轉動解析光譜可以用來研究小行星的表面變化。我們在2011年用鹿林一米望遠鏡上的Hiyoyu光譜儀觀測了12顆小行星。資料分析是用標準的IRAF軟體。我們發現有3顆小行星在觀測期間有顯著的變化。要確定這些變化是否為其表面成分的不同，更多研究是必須的。

摘要(英)

Asteroids are the major members in Solar system quantitatively. The surface composition of asteroids is an important factor to determine their evolutional history as well as their interaction to other Solar system bodies. Rotationally resolved spectroscopy can be used to study the surface variations of asteroids. We used Hiyoyu spectrometer attached to Lulin One-meter telescope to perform observations on 12 asteroids in 2011. Data reduction is done with standard IRAF program. We found three asteroids show significant variation during our observation. Further studies are needed to confirm whether these variations are compositional differences on their surface.

關鍵字(中)

★ 小行星
★ 光譜
★ 轉動解析

關鍵字(英)

★ Asteroids
★ Spectroscopy
★ Rotationally resolved

論文目次

摘要……………………………………………………………………….....................i
Abstract……………………………………………………………………….............. ii
Contents………………………………………………………………………............iii
List of Tables………………………………………………………………………….iv
List of Figures…………………………………………………………………………v
1. Introduction………………………………………………………………………....1
1.1 Photometry and Spectroscopy of Asteroids………………………………….1
1.2 Rotationally Resolved Spectroscopy…………………………………............3
2. Observation…………………………………………………………………………5
2.1 Hiyoyu Spectrometer…………………………………………………………5
2.2 Observation Circumstances…………………………………………………..6
3. Data Analysis……………………………………………………………………...12
3.1 Data Reduction……………………………………………………………...12
3.2 Failed Attempt………………………………………………………………13
3.3 Results………………………………………………………………………14
3.3.1 C-Types……………………………………………………………...14
3.3.1.1 (31) Euphrosyne……………………………………………...14
3.3.1.2 (52) Europa……………………………………………….......15
3.3.1.3 (444) Gyptis………………………………………………......17
3.3.2 S–type………………………………………………..........................19
3.3.2.1 (12) Victoria……………………………………………….....19
3.3.2.2 (27) Euterpe………………………………………………......20
3.3.2.3 (32) Pomona……………………………………………….....22
3.3.2.4 (40) Harmonia………………………………………………..25
3.3.2.5 (43) Ariadne……………………………………………….....27
3.3.2.6 (115) Thyra……………………………………………….......29
3.3.3 M–type………………………………………………........................31
3.3.3.1 (22) Kalliope………………………………………………....31
3.3.3.2 (250) Bettina……………………………………………….....34
3.3.4 E–type………………………………………………..........................36
3.3.4.1 (44) Nysa………………………………………………..........36
4. Discussion………………………………………………........................................40
References………………………………………………............................................41

參考文獻

Barucci, M. A., and Lazzarin, M. 1993, “Koronis family: Reflectance spectra of 243 Ida, 1442 Corvina and 2226 Cunitza”, P&SS, 41, 641-646.
Barruci, M. A. et al. 2008, “Asteroids 2867 Steins and 21 Lutetia: surface composition from far infrared observations with the Spitzer space telescope”, A&A, 477, 665-670.
Bell, J. F. et al. 1988, “The 52-Color Asteroid Survey: Final Results and Interpretation”, abstract of LPSC, 19, 57
Binzel, R. P. et al. 1995, “Rotationally resolved spectra of asteroid 16 Psyche”, Icarus, 117, 443-445.
Birlan, M. et al. 2004, “Near-IR spectroscopy of asteroids 21 Lutetia, 89 Julia, 140 Siwa, 2181 Fogelin and 5480 (1989YK8), potential targets for the Rosetta mission; remote observations campaign on IRTF”, New Astronomy, 9, 343-351.
Campins, H. et al. 2010, “Water ice and organics on the surface of the asteroid 24 Themis”, Nature, 464, 1320-1321.
Feierberg, M. A. et al. 1980, “Spectroscopic evidence for two achondrite parent bodies - Asteroids 349 Dembowska and 4 Vesta”, Geochimica et Cosmochimica Acta, 44, 513-524.
Festou, M. C. et al. 1991, “Asteroid 4 Vesta - Simultaneous visible and ultraviolet IUE observations”, Icarus, 94, 218-231.
Gaffey, M. J. 1984, “Rotational spectral variations of asteroid (8) Flora Implications for the nature of the S-type asteroids and for the parent bodies of the ordinary chondrites”, Icarus, 60, 83-114.
Gaffey, M. J. 1997, “Surface Lithologic Heterogeneity of Asteroid 4 Vesta”, Icarus, 127, 130-157.
Gaffey, M. J., and Gilbert, S. L. 1998, “Asteroid 6 Hebe: The probable parent body of the H-Type ordinary chondrites and the IIE iron meteorites”, M&PS, 33, 1281-1295.
Lagerkvist, C.-I. et al. 1995, “Physical studies of asteroids. XXIX: Photometry and analysis of 27 asteroids”, A&A, 113, 115-129.
Licandro, J., and Pinilla-Alonso, N. 2005, “The Inhomogeneous Surface of Centaur 32522 Thereus (2001 PT13)”, AJ, 630, 93-96.
Lustig, G., and Dvorak, R. 1975, “Photometric investigations of the asteroids (43) Ariadne and (71) Niobe.”, Acta Phys. Austriaca, 43, 89.
Migliorini, F. et al. 1997, “(7) Iris: a possible source of ordinary chondrites?”, A&A, 321, 652-659.
Michalowski, T., and Velichko, F. P. 1990, “Photoelectric photometry, parameters of rotation and shapes of asteroids 22 Kalliope and 79 Eurynome”, Acta Astronomica, 40, 321-332.
Michałowski, T., et al. 2004, “Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona”, A&A, 416, 353
Migliorini, F. et al. 1997, “Surface Properties of (6) Hebe: A Possible Parent Body of Ordinary Chondrites”, Icarus, 128, 104-113.
Mothé-Diniz, T. et al. 2000, “Rotationally Resolved Spectra of Some S-type Asteroids”, Icarus, 148, 494-507.
Mothé-Diniz, T. et al. 2001, “Rotationally Resolved Spectra of 10 Hygiea and a Spectroscopic Study of the Hygiea Family”, Icarus, 152, 117-126.
Murchie, S. L., and Pieters, C. M. 1996, “Spectral properties and rotational spectral heterogeneity of 433 Eros”, Journal of Geophysical Research, 101, 2201-2214.
Nathues, A. et al. 2005, “Spectral study of the Eunomia asteroid family. I. Eunomia”, Icarus, 175, 452-463.
Nedelcu, D. A. et al. 2007, “Near infra-red spectroscopy of the asteroid 21 Lutetia. II. Rotationally resolved spectroscopy of the surface”, A&A, 470, 1157-1164.
Ockert-Bell, M. E. et al. 2008, “Observations of X/M asteroids across multiple wavelengths”, Icarus, 195, 206-219.
Ockert-Bell, M. E. et al. 2010, “The composition of M-type asteroids: Synthesis of spectroscopic and radar observations”, Icarus, 210, 674-692.
Perna, D. et al. 2010, “Inhomogeneities on the surface of 21 Lutetia, the asteroid target of the Rosetta mission. Ground-based results before the Rosetta fly-by”, A&A, 513, 4-6.
Pilcher, F. 2009, “New lightcurves of 8 Flora, 13 Egeria, 14 Irene, 25 Phocaea, 40 Harmonia, 74 Galatea, and 122 Gerda”, Minor Planet Bulletin, 36, 133.
Reddy, V. et al. 2011, “Photometric, spectral phase and temperature effects on 4 Vesta and HED meteorites: Implications for the Dawn mission”, Icarus, 217, 153-168.
Reed, K. L. et al. 1997, “Shape and Albedo Variations of Asteroid 15 Eunomia”, Icarus, 125, 446-454.
Sawyer, S. R. 1991, “A High-Resolution CCD Spectroscopic Survey of Low-Albedo Main Belt Asteroids”, PhD thesis, The University of Texas
Schober, H. J. 1976, “Photoelectric photometry of the minor planet 32 Pomona Composite light curve and the synodic period of rotation”, A&A, 53, 115.
Shepard, M. K. et al. 2008, “Multi-wavelength observations of Asteroid 2100 Ra-Shalom”, Icarus, 193, 20-38.
Shevchenko, V. G. et al. 1992, “Photometry of seventeen asteroids”, Icarus, 100, 295.
Michalowski, T. et al. 2004, “Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona”, A&A, 416, 353.
Takato, N. 2008, “Rotation-Resolved Spectroscopy of a Very Young Asteroid, (1270) Datura”, ApJ, 685, 161-163.
Tanga, P. et al. 2003, "Asteroid observations with the Hubble Space Telescope", A& A, 401, 733–741.
Vernazza, P. et al. 2005, “Analysis of near-IR spectra of 1 Ceres and 4 Vesta, targets of the Dawn mission”, A&A, 436, 1113-1121.
Vilas, F. et al. 1998, “Vilas Asteroid Spectra V1.1.”, NASA Planetary Data System
Zeller, B. et al. 1985, “The eight-color asteroid survey - Results for 589 minor planets”, Icarus, 61, 355-416

指導教授

葉永烜(Wing-Huen Ip)

審核日期

2013-1-21

推文