Evolution of Halley-Type Comets and Meteoroid Streams
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
The Minor Planet Bulletin
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 36, NUMBER 3, A.D. 2009 JULY-SEPTEMBER 77. PHOTOMETRIC MEASUREMENTS OF 343 OSTARA Our data can be obtained from http://www.uwec.edu/physics/ AND OTHER ASTEROIDS AT HOBBS OBSERVATORY asteroid/. Lyle Ford, George Stecher, Kayla Lorenzen, and Cole Cook Acknowledgements Department of Physics and Astronomy University of Wisconsin-Eau Claire We thank the Theodore Dunham Fund for Astrophysics, the Eau Claire, WI 54702-4004 National Science Foundation (award number 0519006), the [email protected] University of Wisconsin-Eau Claire Office of Research and Sponsored Programs, and the University of Wisconsin-Eau Claire (Received: 2009 Feb 11) Blugold Fellow and McNair programs for financial support. References We observed 343 Ostara on 2008 October 4 and obtained R and V standard magnitudes. The period was Binzel, R.P. (1987). “A Photoelectric Survey of 130 Asteroids”, found to be significantly greater than the previously Icarus 72, 135-208. reported value of 6.42 hours. Measurements of 2660 Wasserman and (17010) 1999 CQ72 made on 2008 Stecher, G.J., Ford, L.A., and Elbert, J.D. (1999). “Equipping a March 25 are also reported. 0.6 Meter Alt-Azimuth Telescope for Photometry”, IAPPP Comm, 76, 68-74. We made R band and V band photometric measurements of 343 Warner, B.D. (2006). A Practical Guide to Lightcurve Photometry Ostara on 2008 October 4 using the 0.6 m “Air Force” Telescope and Analysis. Springer, New York, NY. located at Hobbs Observatory (MPC code 750) near Fall Creek, Wisconsin. -
Michael Kühn Detlev Auvermann RARE BOOKS
ANTIQUARIAT 55Michael Kühn Detlev Auvermann RARE BOOKS 1 Rolfinck’s copy ALESSANDRINI, Giulio. De medicina et medico dialogus, libris quinque distinctus. Zurich, Andreas Gessner, 1557. 4to, ff. [6], pp. AUTOLYKOS (AUTOLYCUS OF PYTANE). 356, ff. [8], with printer’s device on title and 7 woodcut initials; a few annotations in ink to the text; a very good copy in a strictly contemporary binding of blind-stamped pigskin, the upper cover stamped ‘1557’, red Autolyci De vario ortu et occasu astrorum inerrantium libri dvo nunc primum de graeca lingua in latinam edges, ties lacking; front-fly almost detached; contemporary ownership inscription of Werner Rolfinck on conuersi … de Vaticana Bibliotheca deprompti. Josepho Avria, neapolitano, interprete. Rome, Vincenzo title (see above), as well as a stamp and duplicate stamp of Breslau University library. Accolti, 1588. 4to, ff. [6], pp. 70, [2]; with large woodcut device on title, and several woodcut diagrams in the text; title a little browned, else a fine copy in 19th-century vellum-backed boards, new endpapers. EUR 3.800.- EUR 4.200.- First edition of Alessandrini’s medical dialogues, his most famous publication and a work of rare erudition. Very rare Latin edition, translated from a Greek manuscript at the Autolycus was a Greek mathematician and astronomer, who probably Giulio Alessandrini (or Julius Alexandrinus de Neustein) (1506–1590) was an Italian physician and author Vatican library, of Autolycus’ work on the rising and setting of the fixed flourished in the second half of the 4th century B.C., since he is said to of Trento who studied philosophy and medicine at the University of Padua, then mathematical science, stars. -
The Comet's Tale
THE COMET’S TALE Journal of the Comet Section of the British Astronomical Association Number 33, 2014 January Not the Comet of the Century 2013 R1 (Lovejoy) imaged by Damian Peach on 2013 December 24 using 106mm F5. STL-11k. LRGB. L: 7x2mins. RGB: 1x2mins. Today’s images of bright binocular comets rival drawings of Great Comets of the nineteenth century. Rather predictably the expected comet of the century Contents failed to materialise, however several of the other comets mentioned in the last issue, together with the Comet Section contacts 2 additional surprise shown above, put on good From the Director 2 appearances. 2011 L4 (PanSTARRS), 2012 F6 From the Secretary 3 (Lemmon), 2012 S1 (ISON) and 2013 R1 (Lovejoy) all Tales from the past 5 th became brighter than 6 magnitude and 2P/Encke, 2012 RAS meeting report 6 K5 (LINEAR), 2012 L2 (LINEAR), 2012 T5 (Bressi), Comet Section meeting report 9 2012 V2 (LINEAR), 2012 X1 (LINEAR), and 2013 V3 SPA meeting - Rob McNaught 13 (Nevski) were all binocular objects. Whether 2014 will Professional tales 14 bring such riches remains to be seen, but three comets The Legacy of Comet Hunters 16 are predicted to come within binocular range and we Project Alcock update 21 can hope for some new discoveries. We should get Review of observations 23 some spectacular close-up images of 67P/Churyumov- Prospects for 2014 44 Gerasimenko from the Rosetta spacecraft. BAA COMET SECTION NEWSLETTER 2 THE COMET’S TALE Comet Section contacts Director: Jonathan Shanklin, 11 City Road, CAMBRIDGE. CB1 1DP England. Phone: (+44) (0)1223 571250 (H) or (+44) (0)1223 221482 (W) Fax: (+44) (0)1223 221279 (W) E-Mail: [email protected] or [email protected] WWW page : http://www.ast.cam.ac.uk/~jds/ Assistant Director (Observations): Guy Hurst, 16 Westminster Close, Kempshott Rise, BASINGSTOKE, Hampshire. -
Aqueous Alteration on Main Belt Primitive Asteroids: Results from Visible Spectroscopy1
Aqueous alteration on main belt primitive asteroids: results from visible spectroscopy1 S. Fornasier1,2, C. Lantz1,2, M.A. Barucci1, M. Lazzarin3 1 LESIA, Observatoire de Paris, CNRS, UPMC Univ Paris 06, Univ. Paris Diderot, 5 Place J. Janssen, 92195 Meudon Pricipal Cedex, France 2 Univ. Paris Diderot, Sorbonne Paris Cit´e, 4 rue Elsa Morante, 75205 Paris Cedex 13 3 Department of Physics and Astronomy of the University of Padova, Via Marzolo 8 35131 Padova, Italy Submitted to Icarus: November 2013, accepted on 28 January 2014 e-mail: [email protected]; fax: +33145077144; phone: +33145077746 Manuscript pages: 38; Figures: 13 ; Tables: 5 Running head: Aqueous alteration on primitive asteroids Send correspondence to: Sonia Fornasier LESIA-Observatoire de Paris arXiv:1402.0175v1 [astro-ph.EP] 2 Feb 2014 Batiment 17 5, Place Jules Janssen 92195 Meudon Cedex France e-mail: [email protected] 1Based on observations carried out at the European Southern Observatory (ESO), La Silla, Chile, ESO proposals 062.S-0173 and 064.S-0205 (PI M. Lazzarin) Preprint submitted to Elsevier September 27, 2018 fax: +33145077144 phone: +33145077746 2 Aqueous alteration on main belt primitive asteroids: results from visible spectroscopy1 S. Fornasier1,2, C. Lantz1,2, M.A. Barucci1, M. Lazzarin3 Abstract This work focuses on the study of the aqueous alteration process which acted in the main belt and produced hydrated minerals on the altered asteroids. Hydrated minerals have been found mainly on Mars surface, on main belt primitive asteroids and possibly also on few TNOs. These materials have been produced by hydration of pristine anhydrous silicates during the aqueous alteration process, that, to be active, needed the presence of liquid water under low temperature conditions (below 320 K) to chemically alter the minerals. -
The Minor Planet Bulletin 37 (2010) 45 Classification for 244 Sita
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 37, NUMBER 2, A.D. 2010 APRIL-JUNE 41. LIGHTCURVE AND PHASE CURVE OF 1130 SKULD Robinson (2009) from his data taken in 2002. There is no evidence of any change of (V-R) color with asteroid rotation. Robert K. Buchheim Altimira Observatory As a result of the relatively short period of this lightcurve, every 18 Altimira, Coto de Caza, CA 92679 (USA) night provided at least one minimum and maximum of the [email protected] lightcurve. The phase curve was determined by polling both the maximum and minimum points of each night’s lightcurve. Since (Received: 29 December) The lightcurve period of asteroid 1130 Skuld is confirmed to be P = 4.807 ± 0.002 h. Its phase curve is well-matched by a slope parameter G = 0.25 ±0.01 The 2009 October-November apparition of asteroid 1130 Skuld presented an excellent opportunity to measure its phase curve to very small solar phase angles. I devoted 13 nights over a two- month period to gathering photometric data on the object, over which time the solar phase angle ranged from α = 0.3 deg to α = 17.6 deg. All observations used Altimira Observatory’s 0.28-m Schmidt-Cassegrain telescope (SCT) working at f/6.3, SBIG ST- 8XE NABG CCD camera, and photometric V- and R-band filters. Exposure durations were 3 or 4 minutes with the SNR > 100 in all images, which were reduced with flat and dark frames. -
Mpc 20051215
2005 DEC. 15 M.P.C. 55685 The MINOR PLANET CIRCULARS/MINOR PLANETS AND COMETS are published, on behalf of Commission 20 of the International Astronomical Union, usually in batches on or near the date of each full moon, by: Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. [email protected] or FAX 617{495{7231 (subscriptions) [email protected] (science) Phone 617{495{7244/7444/7440/7273 (for emergency use only). World-Wide Web address http://cfa-www.harvard.edu/iau/mpc.html ISSN 0736-6884 Brian G. Marsden, Director Gareth V. Williams, Associate Director Timothy B. Spahr, NEO Technical Specialist Syuichi Nakano, Andreas Doppler and Kyle E. Smalley, Associates Supported in part by the Brinson and TABASGO Foundations c Copyright 2005 Minor Planet Center Prepared using the Tamkin Foundation Computer Network ° EDITORIAL NOTICE 147 Osservatorio Astron¶omico di Suno. Observers L. Buzzi, D. Crespi, S. Foglia, G. Galli, S. Minuto, V. Sacco. Measurers L. Buzzi, S. Foglia, G. Galli, The Minor Planet Center is pleased to acknowledge with thanks another gen- S. Minuto. 0.40-m /4 reflector + CCD. erous donation from F. K. Edmondson (Bloomington, IN; senior former president of f 170 Observatorio de Begues. Observer J. Manteca. 0.36-m /10 Schmidt- IAU Commission 20). f Cassegrain + CCD. The next batch of Minor Planet Circulars will be issued on or about 2006 Feb. 201 Jonathan B. Postel Observatory. Observer V. Pozzoli. 0.30-m f/10 reflector 13. There will be no Circulars during January. + CCD. 204 Schiaparelli Observatory. Observer L. -
Kosmos, and Uranus
K O 2 M O 2 : A General £>urbep OF THE PHYSICAL PHENOMENA OF THE UNIVERSE. BY ALEXANDER VON HUMBOLDT. Vol. I. Natune vero rerum vis atque majestaa in omnibus moment is fide caret, si quia modo partes ejus ac non totam compiectatur animo. Pi- in., Hist. Nat. lib. yH. cap. 1. LONDON: HIPPOLYTE BAILLIERE, PUBLISHER, AND FOREIGN BOOKSELLER, 219, REGENT STREET. 1845. TCI HIS MAJESTY THE KING OF PRUSSIA, FREDERICK-WILLIAM IV, THIS SURVEY OF THE PHYSICAL HISTORY OF THE UNIVERSE, 3Jg Betifcatrti, WITH FEELINGS OF DEEP RESPECT AND HEARTFELT GRATITUDE, BY ALEXANDER von HUMBOLDT. PREFACE. In the evening of a long and active life, I present the public with a work the indefinite outlines of which have floated in my mind for almost half a century. I have, in many moods, regarded this work as impracticable; and when I had abandoned it, have still, rashly perhaps, returned to it again. — I lay it before my contemporaries with the diffidence which a reasonable mistrust in the measure ^of my abilities inspires. I also endeavour to forget, that works long looked for are commonly less indulgently received. If circumstances, and an irresistible propensity to pur sue science of various kinds, led me to devote myself for many years, and almost exclusively as it seemed, to parti cular branches, — to descriptive botany, geology, chemistry, astronomical observation and terrestrial magnetism, — as preparatives for a journey on a great scale, the special purpose of my studies was always one still higher than this. My main object was to prepare myself to compre Vlll PREFACE. -
The Minor Planet Bulletin 36, 188-190
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 37, NUMBER 3, A.D. 2010 JULY-SEPTEMBER 81. ROTATION PERIOD AND H-G PARAMETERS telescope (SCT) working at f/4 and an SBIG ST-8E CCD. Baker DETERMINATION FOR 1700 ZVEZDARA: A independently initiated observations on 2009 September 18 at COLLABORATIVE PHOTOMETRY PROJECT Indian Hill Observatory using a 0.3-m SCT reduced to f/6.2 coupled with an SBIG ST-402ME CCD and Johnson V filter. Ronald E. Baker Benishek from the Belgrade Astronomical Observatory joined the Indian Hill Observatory (H75) collaboration on 2009 September 24 employing a 0.4-m SCT PO Box 11, Chagrin Falls, OH 44022 USA operating at f/10 with an unguided SBIG ST-10 XME CCD. [email protected] Pilcher at Organ Mesa Observatory carried out observations on 2009 September 30 over more than seven hours using a 0.35-m Vladimir Benishek f/10 SCT and an unguided SBIG STL-1001E CCD. As a result of Belgrade Astronomical Observatory the collaborative effort, a total of 17 time series sessions was Volgina 7, 11060 Belgrade 38 SERBIA obtained from 2009 August 20 until October 19. All observations were unfiltered with the exception of those recorded on September Frederick Pilcher 18. MPO Canopus software (BDW Publishing, 2009a) employing 4438 Organ Mesa Loop differential aperture photometry, was used by all authors for Las Cruces, NM 88011 USA photometric data reduction. The period analysis was performed using the same program. David Higgins Hunter Hill Observatory The data were merged by adjusting instrumental magnitudes and 7 Mawalan Street, Ngunnawal ACT 2913 overlapping characteristic features of the individual lightcurves. -
The Minor Planet Bulletin Lost a Friend on Agreement with That Reported by Ivanova Et Al
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 33, NUMBER 3, A.D. 2006 JULY-SEPTEMBER 49. LIGHTCURVE ANALYSIS FOR 19848 YEUNGCHUCHIU Kwong W. Yeung Desert Eagle Observatory P.O. Box 105 Benson, AZ 85602 [email protected] (Received: 19 Feb) The lightcurve for asteroid 19848 Yeungchuchiu was measured using images taken in November 2005. The lightcurve was found to have a synodic period of 3.450±0.002h and amplitude of 0.70±0.03m. Asteroid 19848 Yeungchuchiu was discovered in 2000 Oct. by the author at Desert Beaver Observatory, AZ, while it was about one degree away from Jupiter. It is named in honor of my father, The amplitude of 0.7 magnitude indicates that the long axis is Yeung Chu Chiu, who is a businessman in Hong Kong. I hoped to about 2 times that of the shorter axis, as seen from the line of sight learn the art of photometry by studying the lightcurve of 19848 as at that particular moment. Since both the maxima and minima my first solo project. have similar “height”, it’s likely that the rotational axis was almost perpendicular to the line of sight. Using a remote 0.46m f/2.8 reflector and Apogee AP9E CCD camera located in New Mexico Skies (MPC code H07), images of Many amateurs may have the misconception that photometry is a the asteroid were obtained on the nights of 2005 Nov. 20 and 21. very difficult science. After this learning exercise I found that, at Exposures were 240 seconds. -
Implications of Magnitude Distribution Comparisons Between Trans-Neptunian Objects and Comets
Implications of Magnitude Distribution Comparisons between Trans-Neptunian Objects and Comets by Alexander J. Willman, Jr. SpSt 997 “Independent Study” Department of Space Studies University of North Dakota Dr. C. A. Wood, Advisor December 1, 1995 Implications of Magnitude Distribution Comparisons between Trans-Neptunian Objects and Comets Abstract The population of observed trans-neptunian objects has a fairly well-defined magnitude distribution, however, the population of observed short-period comets does not. This analysis of the population distributions of observed trans-neptunian objects (TNOs) and short-period comets (SPCs) indicates that the observed number of TNOs and SPCs is insufficient to judge conclusively whether the trans-neptunian objects are related to the short-period comets or whether the TNOs are part of the Kuiper belt from which the SPCs are believed to be derived. Differences in the population distributions of TNOs and SPCs indicate that the TNOs are not representative of the Kuiper belt as a whole, even if they are part of the Kuiper belt. Further analysis of the population distributions of comets and the TNOs has provided additional information and some predictions about the populations’ characteristics. This derived information includes the facts that: the six brightest SPCs for which H10 magnitudes have been calculated likely belong to the Oort cloud population (long-period) of comets instead of the Kuiper belt population of comets; Pluto and Charon are likely to belong to the TNO population instead of the major planet population; there are likely to be ~109 TNOs in the Kuiper belt, including many Pluto-sized objects, massing a total of ~1025 kg in all. -
The Comet's Tale
THE COMET’S TALE Newsletter of the Comet Section of the British Astronomical Association Volume 8, No 2 (Issue 16), 2001 October DEEP SPACE 1 ENCOUNTERS 19P/Borrelly problem. All the science data ten years to facilitate the five Donald K. Yeomans were successfully received on upcoming cometary encounters Earth within a few hours after the provided by the CONTOUR, NASA/JPL, Near-Earth Object flyby itself. The DS1 spacecraft Stardust, Deep Impact, and program office was designed to test various space Rosetta spacecraft. technologies including the ion On Saturday evening at 7:00 PM, drive engine that first ionizes For more information, see: sustained applause broke out in xenon and then electrostatically the Deep Space 1 spacecraft accelerated these charged http://nmp.jpl.nasa.gov/ds1/ control room at the Jet Propulsion particles to form a modest, but Laboratory. The first high continuous, rocket thrust. resolution images of comet's Borrelly nucleus had reached Earth (Figure 1). The images were sharper than expected and revealed a very dark, outgasing nucleus shaped a bit like a bowling pin except this bowling pin was nearly the size of Mt. Everest. Examination of the surface features reveals ridges, fault lines, and bright areas that are thought to be source regions for the nucleus' jets that emanate toward the solar direction. These Figure 2 This image of comet jets are thought to be the vaporization of the comet's ices as Borrelly's nucleus has been the active regions are heated by Figure 1 This black and white purposely overexposed to show sunlight (Figure 2). -
The Astronomer Magazine Index
The Astronomer Magazine Index The numbers in brackets indicate approx lengths in pages (quarto to 1982 Aug, A4 afterwards) 1964 May p1-2 (1.5) Editorial (Function of CA) p2 (0.3) Retrospective meeting after 2 issues : planned date p3 (1.0) Solar Observations . James Muirden , John Larard p4 (0.9) Domes on the Mare Tranquillitatis . Colin Pither p5 (1.1) Graze Occultation of ZC620 on 1964 Feb 20 . Ken Stocker p6-8 (2.1) Artificial Satellite magnitude estimates : Jan-Apr . Russell Eberst p8-9 (1.0) Notes on Double Stars, Nebulae & Clusters . John Larard & James Muirden p9 (0.1) Venus at half phase . P B Withers p9 (0.1) Observations of Echo I, Echo II and Mercury . John Larard p10 (1.0) Note on the first issue 1964 Jun p1-2 (2.0) Editorial (Poor initial response, Magazine name comments) p3-4 (1.2) Jupiter Observations . Alan Heath p4-5 (1.0) Venus Observations . Alan Heath , Colin Pither p5 (0.7) Remarks on some observations of Venus . Colin Pither p5-6 (0.6) Atlas Coeli corrections (5 stars) . George Alcock p6 (0.6) Telescopic Meteors . George Alcock p7 (0.6) Solar Observations . John Larard p7 (0.3) R Pegasi Observations . John Larard p8 (1.0) Notes on Clusters & Double Stars . John Larard p9 (0.1) LQ Herculis bright . George Alcock p10 (0.1) Observations of 2 fireballs . John Larard 1964 Jly p2 (0.6) List of Members, Associates & Affiliations p3-4 (1.1) Editorial (Need for more members) p4 (0.2) Summary of June 19 meeting p4 (0.5) Exploding Fireball of 1963 Sep 12/13 .