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TOPIC: Trans-Neptunian objects


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RE: Trans-Neptunian objects
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I am working with solar system research. My main research interests are: trans-Neptunian objects (in the trans-Neptunian belt or Edgeworth-Kuiper belt), small solar system bodies, Centaurs, Trojans, orbital resonances, planet formation and migration and dynamics of minor bodies in general. Right now I am a JSPS fellow working at Kobe University.
Patryk Sofia Lykawka




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Title: An Outer Planet Beyond Pluto and Origin of the Trans-Neptunian Belt Architecture
Authors: Patryk Sofia Lykawka, Tadashi Mukai

Trans-Neptunian objects (TNOs) are remnants of a collisionally and dynamically evolved planetesimal disk in the outer solar system. This complex structure, known as the trans-Neptunian belt (or Edgeworth-Kuiper belt), can reveal important clues about disk properties, planet formation, and other evolutionary processes. In contrast to the predictions of accretion theory, TNOs exhibit surprisingly large eccentricities, e, and inclinations, i, which can be grouped into distinct dynamical classes. Several models have addressed the origin and orbital evolution of TNOs, but none have reproduced detailed observations, e.g., all dynamical classes and peculiar objects, or provided insightful predictions. Based on extensive simulations of planetesimal disks with the presence of the four giant planets and massive planetesimals, we propose that the orbital history of an outer planet with tenths of Earth's mass can explain the trans-Neptunian belt orbital structure. This massive body was likely scattered by one of the giant planets, which then stirred the primordial planetesimal disk to the levels observed at 40-50 AU and truncated it at about 48 AU before planet migration. The outer planet later acquired an inclined stable orbit (>100 AU; 20-40 deg) because of a resonant interaction with Neptune (an r:1 or r:2 resonance possibly coupled with the Kozai mechanism), guaranteeing the stability of the trans-Neptunian belt. Our model consistently reproduces the main features of each dynamical class with unprecedented detail; it also satisfies other constraints such as the current small total mass of the trans-Neptunian belt and Neptune's current orbit at 30.1 AU. We also provide observationally testable predictions.

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(145453) 2005 RR43
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Title: The water ice rich surface of (145453) 2005 RR43: a case for a carbon-depleted population of TNOs?
Authors: N. Pinilla-Alonso (1), J. Licandro (2,3), R. Gil-Hutton (4), R. Brunetto (5,6) ((1) Fundacion Galileo Galilei, (2) Isaac Newton Group, (3) Instituto de Astrofisica de Canarias, (4) Complejo Astronomico el Leoncito, (5) Dipartamento di Fisica, Universita di Lecce, (6) INAF-Osservatorio Astrofisico di Catania)
(Version v2)

Recent results suggest that there is a group of TNOs (2003 EL61 being the biggest member), with surfaces composed of almost pure water ice and with very similar orbital elements. We study the surface composition of another TNO that moves in a similar orbit, 2005 RR43, and compare it with the surface composition of the other members of this group. We report visible and near-infrared spectra, obtained with the 4.2m William Herschel Telescope and the 3.58m Telescopio Nazionale Galileo at the "Roque de los Muchachos" Observatory (La Palma, Spain). The spectrum of 2005 RR43 is neutral in colour in the visible and dominated by very deep water ice absorption bands in the near infrared (D= 70.3 2.1 % and 82.8 4.9 % at 1.5 \mu and 2.0 \mu respectively). It is very similar to the spectrum of the group of TNOs already mentioned. All of them present much deeper water ice absorption bands (D>40 %) than any other TNO except Charon. Scattering models show that its surface is covered by water ice, a significant fraction in crytalline state with no trace (5 % upper limit) of complex organics. Possible scenarios to explain the existence of this population of TNOs are discussed: a giant collision, an originally carbon depleted composition, or a common process of continuous resurfacing. We conclude that TNO 2005 RR43 is member of a group, may be a population, of TNOs clustered in the space of orbital parameters that show abundant water ice and no signs of complex organics. The lack of complex organics in their surfaces suggests a significant smaller fraction of carbonaceous volatiles like CH4 in this population than in "normal" TNOs. A carbon depleted population of TNOs could be the origin of the population of carbon depleted Jupiter family comets already noticed by A'Hearn et al. (1995).

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Title: Search for Small Trans-Neptunian Objects by the TAOS Project
Authors: W. P. Chen, C. Al****, T. Axelrod, F. B. Bianco, Y. I. Byun, Y. H. Chang, K. H. Cook, R. Dave, J. Giammarco, D. W. Kim, S. K. King, T. Lee, M. Lehner, C. C. Lin, H. C. Lin, J. J. Lissauer, S. Marshall, N. Meinshausen, S. Mondal, I. de Pater, R. Porrata, J. Rice, M. E. Schwamb, A. Wang, S. Y. Wang, C. Y. Wen, Z. W. Zhang

The Taiwan-America Occultation Survey (TAOS) aims to determine the number of small icy bodies in the outer reach of the Solar System by means of stellar occultation. An array of 4 robotic small (D=0.5 m), wide-field (f/1.9) telescopes have been installed at Lulin Observatory in Taiwan to simultaneously monitor some thousand of stars for such rare occultation events. Because a typical occultation event by a TNO a few km across will last for only a fraction of a second, fast photometry is necessary. A special CCD readout scheme has been devised to allow for stellar photometry taken a few times per second. Effective analysis pipelines have been developed to process stellar light curves and to correlate any possible flux changes among all telescopes. A few billion photometric measurements have been collected since the routine survey began in early 2005. Our preliminary result of a very low detection rate suggests a deficit of small TNOs down to a few km size, consistent with the extrapolation of some recent studies of larger (30--100 km) TNOs.

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Title: Solar System: Sifting through the debris
Authors: Asantha Cooray (UC Irvine)

A quadrillion previously unnoticed small bodies beyond Neptune have been spotted as they dimmed X-rays from a distant source. Models of the dynamics of debris in the Solar System's suburbs must now be reworked.

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Title: Occultation of X-rays from Scorpius X-1 by small trans-neptunian objects
Authors: Hsiang-Kuang Chang1,2, Sun-Kun King3, Jau-Shian Liang1, Ping-Shien Wu2, Lupin Chun-Che Lin1 and Jeng-Lun Chiu1

Since the first discovery of the Trans-Neptunian Objects (TNOs) in 1992, nearly one thousand new members have been added to our solar system, among which several are of size comparable to or even larger than Pluto. Their population properties such as the size distribution and the total number are valuable information for understanding the formation of the solar system. Because TNOs are distant and small, direct detection is only possible for larger ones with diameter above several tens of kilometres. For smaller ones, which are expected to be more abundant in number, occultation of background stars by TNOs as a way to study their properties has been proposed but without any definite detection so far. Here we report the discovery of such occultation events at millisecond time scales in the X-ray light curve of Scorpius X-1. Assumed to be at a heliocentric distance of 43 AU in a circular Keplerian orbital motion, these occulting TNOs are estimated to have sizes about or less than 100 m. This is the first time that TNOs of such a small size are detected. Their abundance is in line with an extrapolation from the size distribution of TNOs larger than 100 km, without showing any indication of a possible turnover predicted by coagulation models for planet formation with collisional erosion. Diffraction patterns in the occultation light curves may provide further information to better determine the distances of these occulting TNOs.

Source (Doc)

The small trans-neptunian objects in our solar system were found by observations of the star Scorpius X-1 (Sco X1), by the Rossi X-ray Timing Explorer satellite.

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Title: The Diverse Solar Phase Curves of Distant Icy Bodies. Part I: Photometric Observations of 18 Trans-Neptunian Objects, 7 Centaurs, and Nereid
Authors: David L. Rabinowitz (Yale), Bradley E. Schaefer (LSU), Suzanne W. Tourtellotte (Yale)

Researchers have measured the solar phase curves in B, V, and I for 18 Trans-Neptunian Objects, 7 Centaurs, and Nereid and determined the rotation curves for 10 of these targets.
For each body, they have made ~100 observations uniformly spread over the entire visible range.
They find that all the targets except Nereid have linear phase curves at small phase angles (< 2 deg) with widely varying phase coefficients (0.0 to 0.4 mag/deg). At phase angles > 3 deg, the Centaurs (54598) Bienor and (32532) Thereus have phase curves that flatten.
The recently discovered Pluto-scale bodies (2003 UB313, 2005 FY9, and 2003 EL61), like Pluto, have neutral colours compared to most TNOs and small phase coefficients (< 0.1 mag/deg). Together these two properties are a likely indication for large TNOs of high-albedo, freshly coated icy surfaces. The researchers find several bodies with significantly wavelength-dependent phase curves.
The TNOs (50000) Quaoar, (120348) 2004 TY364 (47932), and 2000 GN171 have unusually high I-band phase coefficients (0.2900.038, 0.4130.064, 0.2810.033 mag/deg, respectively) and much lower coefficients in the B and V bands. Their phase coefficients increase in proportion to wavelength by 0.5 - 0.8 mag/deg/um. The phase curves for TNOs with small B-band phase coefficients (< 0.1 mag/deg) have a similar but weaker wavelength dependence. Coherent backscatter is the likely cause for the wavelength dependence for all these bodies. They see no such dependence for the Centaurs, which have visual albedos ~0.05.

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Astronomers have found 45 previously unknown bodies of rock and ice orbiting beyond Neptune in the Kuiper Belt. They range from about 50 to 500 kilometres wide.

The announcement is probably a record for the most new solar system objects reported simultaneously, increasing the number of distant objects with well defined orbits by nearly 10%.
But its real importance will be in measuring the distribution of distant objects well enough to test theories of how the outer solar system evolved.

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K04FG4W C2004 04 15.38135 13 06 41.76 -07 02 05.0 EH029675
K04FG4W C2004 04 16.24938 13 06 37.08 -07 01 32.4 EH029675
K04FG4W C2004 05 24.19250 13 03 43.16 -06 41 31.6 EH029695
K04FG4W C2004 05 24.24012 13 03 43.01 -06 41 30.8 EH029695
K04FG4W C2004 05 24.29308 13 03 42.83 -06 41 29.3 EH029695
K04FG4W C2005 07 08.28030 13 10 46.54 -07 01 35.5 22.9 r EH029568
K04FG4W C2005 08 01.97568 13 11 43.10 -07 06 17.5 EH029309
K04FG4W C2005 08 01.97898 13 11 43.12 -07 06 17.8 EH029309
K04FG4W C2005 08 01.98307 13 11 43.12 -07 06 17.8 EH029309
K04FG4W C2005 08 02.97488 13 11 46.72 -07 06 37.3 EH029309
K04FG4W C2005 08 02.97822 13 11 46.72 -07 06 37.8 EH029309
K04FG4W C2005 08 02.98225 13 11 46.73 -07 06 37.4 EH029309
K04XJ0X C2003 12 16.32636 04 41 50.45 +22 13 51.2 23.0 g EH029568
K04XJ0X C2003 12 16.35282 04 41 50.30 +22 13 50.9 23.1 g EH029568
K04XJ0X C2003 12 16.37913 04 41 50.15 +22 13 50.8 23.0 g EH029568
K04XJ0X* C2004 12 11.37599 04 48 31.03 +22 28 11.9 22.9 r EH029568
K04XJ0X C2004 12 11.40470 04 48 30.87 +22 28 11.7 22.7 r EH029568
K04XJ0X C2004 12 11.43762 04 48 30.69 +22 28 11.5 22.6 r EH029568
K04XJ0X C2004 12 12.29935 04 48 26.08 +22 28 03.7 22.7 r EH029568
K04XJ0X C2005 10 03.44035 04 59 38.46 +22 47 36.1 22.7 R EH029675
K04XJ0X C2005 10 03.48273 04 59 38.38 +22 47 36.0 EH029675
K04XJ0X C2005 10 04.40111 04 59 36.83 +22 47 34.3 EH029675
K04XJ0X C2005 10 04.45446 04 59 36.73 +22 47 34.0 EH029675
K04XJ0X C2005 12 04.37664 04 55 28.66 +22 41 53.0 23.0 r EH029697
K04XJ0X C2005 12 04.41527 04 55 28.46 +22 41 53.0 23.1 r EH029697
K04XJ0X C2005 12 05.36885 04 55 23.23 +22 41 44.9 23.5 r EH029697
K04XJ0X C2005 12 05.41756 04 55 22.97 +22 41 44.3 23.0 r EH029697
K04XJ0X C2005 12 06.37454 04 55 17.81 +22 41 37.2 22.9 r EH029697
K04XJ0X C2005 12 06.42560 04 55 17.50 +22 41 36.8 23.2 r EH029697
K05TI9V C2003 12 16.31490 04 08 59.57 +21 52 44.3 22.8 g EH029568
K05TI9V C2003 12 16.34141 04 08 59.39 +21 52 43.7 22.9 g EH029568
K05TI9V C2003 12 16.36772 04 08 59.20 +21 52 42.9 22.7 g EH029568
K05TI9V C2003 12 17.41945 04 08 52.71 +21 52 12.3 EH029568
K05TI9V C2004 09 12.43791 04 25 17.00 +21 35 37.0 EH029695
K05TI9V C2004 09 13.47709 04 25 16.57 +21 35 23.3 EH029695
K05TI9V* C2005 10 03.41354 04 33 13.79 +20 32 57.8 EH029675
K05TI9V C2005 10 03.46371 04 33 13.65 +20 32 56.7 EH029675
K05TI9V C2005 10 04.38417 04 33 11.08 +20 32 37.9 22.8 R EH029675
K05TI9V C2005 10 04.43375 04 33 10.93 +20 32 36.7 22.9 R EH029675
K05TI9V C2005 11 04.43340 04 30 52.30 +20 20 17.6 22 R EH029695
K05TI9V C2005 11 04.46770 04 30 52.11 +20 20 16.7 22 R EH029695


Orbital elements:

This is the result of a four year search by French and Canadian researchers using the Canada-France-Hawaii Telescope (CFHT) atop Mauna Kea, Hawaii

-- Edited by Blobrana at 01:57, 2006-04-24

__________________


L

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K03SV7O C2004 09 21.40952 00 16 10.38 +02 07 49.6 23.5 r EH029568
K03SV7O C2004 09 21.44066 00 16 10.19 +02 07 48.3 23.5 r EH029568
K03SV7O C2004 09 21.46948 00 16 10.04 +02 07 47.2 23.3 r EH029568
K03SV7O C2004 09 22.41446 00 16 04.82 +02 07 10.3 23.6 r EH029568
K03SV7O C2004 12 03.24625 00 11 10.51 +01 31 54.0 23.4 i EH029568
K03SV7O C2004 12 03.29858 00 11 10.44 +01 31 53.3 23.6 i EH029568
K03SV7O C2005 07 08.55589 00 28 10.23 +03 12 36.4 22.8 r EH029568
K03SV7O C2005 07 08.61960 00 28 10.24 +03 12 36.4 22.5 r EH029568
K03SV7O C2005 07 09.44999 00 28 10.43 +03 12 35.5 EH029675
K03SV7O C2005 07 09.58999 00 28 10.39 +03 12 36.2 22.7 r EH029568
K03SV7O C2005 07 10.46001 00 28 10.55 +03 12 34.0 EH029675
K03SV7P* C2003 09 25.40375 23 28 55.50 -02 52 28.1 EH029568
K03SV7P C2003 09 25.46139 23 28 55.26 -02 52 29.5 EH029568
K03SV7P C2003 09 25.52378 23 28 55.01 -02 52 31.3 EH029568
K03SV7P C2003 09 27.36229 23 28 47.40 -02 53 18.2 23.6 g EH029568
K03SV7P C2003 09 27.41465 23 28 47.19 -02 53 19.4 23.8 g EH029568
K03SV7P C2003 09 27.46965 23 28 46.96 -02 53 20.7 23.2 g EH029568
K03SV7P C2004 09 07.34130 23 34 26.62 -02 10 12.5 22.5 R EH029695
K03SV7P C2004 09 07.42784 23 34 26.25 -02 10 14.8 22.2 R EH029695
K03SV7P C2004 09 11.32843 23 34 09.84 -02 11 55.8 EH029695
K03SV7P C2004 09 11.37361 23 34 09.66 -02 11 57.0 EH029695
K03SV7P C2004 09 11.41886 23 34 09.48 -02 11 58.2 EH029695
K03SV7P C2005 07 08.53283 23 41 46.23 -01 17 31.1 22.8 r EH029568
K03SV7P C2005 07 08.58383 23 41 46.16 -01 17 31.4 23.1 r EH029568
K03SV7P C2005 07 09.55654 23 41 45.11 -01 17 36.4 22.8 r EH029568
K03SV7P C2005 10 03.23850 23 36 59.07 -01 46 15.1 23.0 R EH029675
K03SV7P C2005 10 04.23386 23 36 55.06 -01 46 40.1 EH029675
K03SV7Q* C2003 09 25.40797 23 40 49.56 -01 24 29.0 EH029568
K03SV7Q C2003 09 25.46558 23 40 49.29 -01 24 31.2 EH029568
K03SV7Q C2003 09 27.36654 23 40 40.64 -01 25 42.8 22.4 g EH029568
K03SV7Q C2003 09 27.41890 23 40 40.40 -01 25 44.8 22.2 g EH029568
K03SV7Q C2003 09 27.47452 23 40 40.13 -01 25 46.9 22.6 g EH029568
K03SV7Q C2003 11 22.25748 23 37 37.76 -01 53 20.5 22.8 g EH029568
K03SV7Q C2003 11 22.30824 23 37 37.70 -01 53 21.0 22.6 g EH029568
K03SV7Q C2003 11 22.35785 23 37 37.63 -01 53 21.7 22.6 g EH029568
K03SV7Q C2004 09 06.33357 23 48 24.97 -01 21 28.1 21.6 R EH029695
K03SV7Q C2004 09 06.42332 23 48 24.57 -01 21 31.4 21.7 R EH029695
K03SV7Q C2004 09 07.37809 23 48 20.28 -01 22 06.9 21.7 R EH029695
K03SV7Q C2004 09 11.32051 23 48 02.37 -01 24 35.1 EH029695
K03SV7Q C2004 09 11.36595 23 48 02.18 -01 24 36.6 EH029695
K03SV7Q C2004 09 11.41131 23 48 01.95 -01 24 38.7 EH029695
K03SV7Q C2005 07 08.53895 23 57 27.83 -01 02 32.5 22.0 r EH029568
K03SV7Q C2005 07 08.59476 23 57 27.80 -01 02 33.2 21.8 r EH029568
K03SV7Q C2005 07 09.56507 23 57 27.17 -01 02 46.2 21.8 r EH029568
K03SV7R* C2003 09 25.40797 23 41 20.95 -01 56 07.8 EH029568
K03SV7R C2003 09 25.46558 23 41 20.64 -01 56 09.9 EH029568
K03SV7R C2003 09 27.36654 23 41 11.03 -01 57 17.6 22.9 g EH029568
K03SV7R C2003 09 27.41890 23 41 10.75 -01 57 19.3 23.6 g EH029568
K03SV7R C2003 09 27.47452 23 41 10.47 -01 57 21.6 23.4 g EH029568
K03SV7R C2003 11 22.25748 23 37 49.20 -02 21 44.0 23.0 g EH029568
K03SV7R C2003 11 22.35785 23 37 49.04 -02 21 45.4 22.7 g EH029568
K03SV7R C2004 09 07.39052 23 49 48.60 -01 17 40.5 22.6 R EH029695
K03SV7R C2004 09 07.44022 23 49 48.32 -01 17 42.3 22.6 R EH029695
K03SV7R C2004 09 11.33580 23 49 28.86 -01 19 59.5 EH029695
K03SV7R C2004 09 11.38128 23 49 28.63 -01 20 01.4 EH029695
K03SV7R C2004 09 11.42642 23 49 28.41 -01 20 03.2 EH029695
K03SV7R C2005 07 08.54462 23 59 54.76 -00 25 44.1 22.2 r EH029568
K03SV7R C2005 07 08.60062 23 59 54.72 -00 25 44.5 22.2 r EH029568
K03SV7R C2005 07 10.45526 23 59 53.44 -00 25 59.6 EH029675
K03SV7R C2005 07 11.46556 23 59 52.62 -00 26 08.8 EH029675
K03SV7S C2003 09 25.40797 23 39 54.14 -01 51 17.1 EH029568
K03SV7S* C2003 09 25.46558 23 39 53.77 -01 51 19.7 EH029568
K03SV7S C2003 09 27.36654 23 39 42.10 -01 52 40.8 22.3 g EH029568
K03SV7S C2003 09 27.41890 23 39 41.77 -01 52 43.0 22.1 g EH029568
K03SV7S C2003 09 27.47452 23 39 41.42 -01 52 45.4 21.9 g EH029568
K03SV7S C2003 11 22.25748 23 35 43.07 -02 21 35.2 21.5 g EH029568
K03SV7S C2003 11 22.30824 23 35 42.98 -02 21 35.8 21.5 g EH029568
K03SV7S C2003 11 22.35785 23 35 42.89 -02 21 36.2 21.5 g EH029568
K03SV7S C2004 09 06.34646 23 52 18.85 -00 48 24.6 21.7 R EH029695
K03SV7S C2004 09 06.43654 23 52 18.30 -00 48 28.2 21.6 R EH029695
K03SV7S C2004 09 11.34360 23 51 48.48 -00 51 57.0 EH029695
K03SV7S C2004 09 11.38863 23 51 48.20 -00 51 58.9 EH029695
K03SV7S C2004 09 11.43427 23 51 47.90 -00 52 01.0 EH029695
K03SV7S C2005 07 08.56169 00 06 24.02 +00 27 56.0 20.6 r EH029568
K03SV7S C2005 07 09.45557 00 06 23.76 +00 27 50.8 EH029675
K03SV7S C2005 07 09.59940 00 06 23.68 +00 27 50.1 20.8 r EH029568
K03SV7S C2005 07 10.46398 00 06 23.32 +00 27 44.4 EH029675
K03T58G* C2003 10 03.44381 04 21 58.41 +22 23 40.3 22.7 R EH029568
K03T58G C2003 10 03.49497 04 21 58.29 +22 23 40.0 22.6 R EH029568
K03T58G C2003 10 03.55616 04 21 58.14 +22 23 39.8 22.7 R EH029568
K03T58G C2003 12 16.31653 04 16 39.60 +22 11 06.5 23.1 g EH029568
K03T58G C2003 12 16.34304 04 16 39.47 +22 11 06.2 23.3 g EH029568
K03T58G C2003 12 16.36935 04 16 39.34 +22 11 05.8 23.0 g EH029568
K03T58G C2003 12 17.42108 04 16 34.33 +22 10 52.8 EH029568
K03T58G C2004 12 11.36465 04 22 29.27 +22 23 03.0 22.9 r EH029568
K03T58G C2004 12 11.39348 04 22 29.11 +22 23 02.7 22.7 r EH029568
K03T58G C2004 12 11.42295 04 22 28.96 +22 23 02.3 22.8 r EH029568
K03T58G C2004 12 12.28804 04 22 24.70 +22 22 51.7 23.0 r EH029568
K03T58G C2005 10 04.39000 04 32 51.85 +22 43 38.1 22.5 R EH029675
K03T58G C2005 10 04.44031 04 32 51.73 +22 43 37.8 22.6 R EH029675
K03T58G C2005 10 04.48140 04 32 51.65 +22 43 37.7 22.6 R EH029675
K03T58G C2005 10 04.52268 04 32 51.55 +22 43 37.5 EH029675
K03T58G C2005 11 04.39531 04 31 04.98 +22 40 09.1 22.5 R EH029697
K03T58G C2005 11 04.41985 04 31 04.90 +22 40 08.9 22.5 R EH029697
K03T58G C2005 11 04.44803 04 31 04.75 +22 40 08.5 22.5 R EH029697
K03T58H* C2003 10 03.45706 04 40 42.78 +22 44 53.0 22.8 i EH029568
K03T58H C2003 10 03.50790 04 40 42.66 +22 44 52.4 22.7 i EH029568
K03T58H C2003 10 03.56923 04 40 42.50 +22 44 51.7 22.7 i EH029568
K03T58H C2003 12 16.32472 04 34 30.89 +22 22 52.7 22.5 g EH029568
K03T58H C2003 12 16.35119 04 34 30.73 +22 22 52.0 22.4 g EH029568
K03T58H C2003 12 16.37749 04 34 30.57 +22 22 51.5 22.5 g EH029568
K03T58H C2003 12 17.39650 04 34 24.53 +22 22 30.5 EH029568
K03T58H C2003 12 17.42928 04 34 24.33 +22 22 29.9 EH029568
K03T58H C2004 09 11.48953 04 48 12.81 +22 11 08.8 EH029695
K03T58H C2004 09 12.48215 04 48 13.13 +22 11 00.9 EH029695
K03T58H C2004 09 16.47160 04 48 13.21 +22 10 26.6 EH029675
K03T58H C2004 09 17.46085 04 48 12.92 +22 10 17.6 EH029675
K03T58H C2004 09 18.43761 04 48 12.53 +22 10 08.5 EH029675
K03T58H C2005 11 04.48734 04 53 03.70 +21 20 46.7 22.5 R EH029695
K03T58H C2005 11 04.52093 04 53 03.47 +21 20 46.3 22.5 R EH029695
K03T58H C2005 11 05.51394 04 52 58.52 +21 20 28.8 22.5 R EH029695
K03T58J* C2003 10 03.46019 04 45 05.02 +22 52 18.3 23.0 i EH029568
K03T58J C2003 10 03.51093 04 45 04.92 +22 52 18.1 23.7 i EH029568
K03T58J C2003 10 03.57232 04 45 04.79 +22 52 18.0 23.1 i EH029568
K03T58J C2003 12 16.32636 04 39 40.38 +22 42 59.8 23.5 g EH029568
K03T58J C2003 12 16.35282 04 39 40.24 +22 42 59.4 23.5 g EH029568
K03T58J C2003 12 16.37913 04 39 40.10 +22 42 59.1 23.6 g EH029568
K03T58J C2003 12 17.43092 04 39 34.53 +22 42 48.3 EH029568
K03T58J C2005 12 04.36834 04 53 20.01 +23 09 13.4 23.5 r EH029697
K03T58J C2005 12 04.39627 04 53 19.83 +23 09 13.0 23.6 r EH029697
K03T58J C2005 12 04.43534 04 53 19.63 +23 09 12.9 23.4 r EH029697
K03T58J C2005 12 06.36627 04 53 09.07 +23 08 56.4 23.5 r EH029697
K03T58J C2006 01 28.27637 04 49 09.54 +23 02 13.0 EH029675
K03T58J C2006 01 29.14157 04 49 07.19 +23 02 08.9 EH029675
K03T58K* C2003 10 03.46317 04 48 58.57 +22 44 21.7 23.6 i EH029568
K03T58K C2003 10 03.51380 04 48 58.47 +22 44 21.6 23.4 i EH029568
K03T58K C2003 10 03.57522 04 48 58.36 +22 44 21.3 23.4 i EH029568
K03T58K C2003 12 16.32799 04 44 03.15 +22 36 47.4 23.6 g EH029568
K03T58K C2003 12 16.35445 04 44 03.03 +22 36 47.2 23.6 g EH029568
K03T58K C2003 12 16.38076 04 44 02.91 +22 36 47.0 23.8 g EH029568
K03T58K C2003 12 17.43258 04 43 57.81 +22 36 38.6 EH029568
K03T58K C2004 12 11.37599 04 49 19.86 +22 50 01.9 23.6 r EH029568
K03T58K C2004 12 11.40470 04 49 19.72 +22 50 01.8 23.6 r EH029568
K03T58K C2004 12 11.43762 04 49 19.56 +22 50 01.4 23.4 r EH029568
K03T58K C2004 12 12.29935 04 49 15.30 +22 49 54.9 23.6 r EH029568
K03T58K C2005 11 04.49378 04 57 11.00 +23 06 03.4 23.5 R EH029695
K03T58K C2005 11 04.52749 04 57 10.87 +23 06 03.2 EH029695
K03T58K C2005 11 06.44880 04 57 03.01 +23 05 53.5 23.5 R EH029695
K03T58L* C2003 10 03.46317 04 49 44.25 +22 48 50.2 23.0 i EH029568
K03T58L C2003 10 03.51380 04 49 44.16 +22 48 49.9 EH029568
K03T58L C2003 10 03.57522 04 49 44.04 +22 48 49.7 23.0 i EH029568
K03T58L C2003 12 16.32799 04 44 31.59 +22 37 49.7 23.5 g EH029568
K03T58L C2003 12 16.35445 04 44 31.45 +22 37 49.4 23.4 g EH029568
K03T58L C2003 12 16.38076 04 44 31.31 +22 37 49.1 23.6 g EH029568
K03T58L C2003 12 17.39975 04 44 26.03 +22 37 37.5 EH029568
K03T58L C2003 12 17.43258 04 44 25.89 +22 37 37.1 EH029568
K03T58L C2004 12 11.37788 04 50 48.98 +22 37 40.4 23.0 r EH029568
K03T58L C2004 12 11.40659 04 50 48.83 +22 37 40.1 23.0 r EH029568
K03T58L C2004 12 11.43951 04 50 48.65 +22 37 39.8 23.3 r EH029568
K03T58L C2004 12 12.30124 04 50 44.14 +22 37 30.9 23.2 r EH029568
K03T58L C2005 10 04.41476 05 01 24.71 +22 44 46.9 EH029675
K03T58L C2005 10 04.46827 05 01 24.63 +22 44 46.4 EH029675
K03T58L C2005 10 04.50969 05 01 24.55 +22 44 45.9 22.8 R EH029675
K03YH9J* C2003 12 16.31818 04 19 24.41 +22 18 22.3 23.2 g EH029568
K03YH9J C2003 12 16.34467 04 19 24.26 +22 18 21.9 23.3 g EH029568
K03YH9J C2003 12 16.37098 04 19 24.12 +22 18 21.6 23.5 g EH029568
K03YH9J C2003 12 17.39000 04 19 18.87 +22 18 08.8 EH029568
K03YH9J C2003 12 17.42270 04 19 18.68 +22 18 08.9 EH029568
K03YH9J C2004 12 11.36654 04 26 09.54 +22 35 46.8 22.5 r EH029568
K03YH9J C2004 12 11.39535 04 26 09.38 +22 35 46.5 22.6 r EH029568
K03YH9J C2004 12 11.42484 04 26 09.22 +22 35 46.1 22.6 r EH029568
K03YH9J C2004 12 12.28992 04 26 04.61 +22 35 35.9 22.6 r EH029568
K03YH9J C2005 10 04.42174 04 37 42.86 +23 00 42.8 EH029675
K03YH9J C2005 10 04.47528 04 37 42.74 +23 00 42.7 22.8 R EH029675
K03YH9J C2005 10 04.51629 04 37 42.65 +23 00 42.5 EH029675
K03YH9J C2005 11 04.42651 04 35 51.27 +22 57 42.8 22 R EH029695
K03YH9J C2005 11 04.46117 04 35 51.10 +22 57 42.7 22 R EH029695
K03YH9K C2003 10 03.44690 04 29 32.48 +22 35 09.7 24.3 i EH029568
K03YH9K C2003 10 03.49804 04 29 32.38 +22 35 09.2 24.0 i EH029568
K03YH9K C2003 10 03.55925 04 29 32.23 +22 35 08.9 24.0 i EH029568
K03YH9K* C2003 12 16.31981 04 24 08.17 +22 18 23.8 23.4 g EH029568
K03YH9K C2003 12 16.34630 04 24 08.04 +22 18 23.1 23.4 g EH029568
K03YH9K C2003 12 16.37261 04 24 07.92 +22 18 22.9 23.9 g EH029568
K03YH9K C2003 12 17.39162 04 24 02.87 +22 18 07.1 EH029568
K03YH9K C2004 12 11.36844 04 29 58.90 +22 05 15.4 23.7 r EH029568
K03YH9K C2004 12 11.39721 04 29 58.75 +22 05 15.1 23.8 r EH029568
K03YH9K C2004 12 11.42672 04 29 58.60 +22 05 14.7 24.0 r EH029568
K03YH9K C2005 11 04.44006 04 38 37.26 +21 59 07.0 23.5 R EH029695
K03YH9K C2005 11 04.47426 04 38 37.11 +21 59 06.5 23.5 R EH029695
K03YH9L* C2003 12 16.32309 04 30 23.83 +22 24 22.0 23.2 g EH029568
K03YH9L C2003 12 16.34956 04 30 23.69 +22 24 21.9 22.8 g EH029568
K03YH9L C2003 12 16.37586 04 30 23.54 +22 24 21.6 23.3 g EH029568
K03YH9L C2003 12 17.39487 04 30 17.94 +22 24 08.5 EH029568
K03YH9L C2004 12 11.37032 04 37 23.58 +22 34 43.8 23.3 r EH029568
K03YH9L C2004 12 11.39908 04 37 23.40 +22 34 43.5 23.1 r EH029568
K03YH9L C2004 12 11.42862 04 37 23.23 +22 34 43.1 23.0 r EH029568
K03YH9L C2004 12 12.29368 04 37 18.36 +22 34 32.8 23.2 r EH029568
K03YH9L C2005 10 04.40775 04 49 13.78 +22 52 41.0 23.0 R EH029675
K03YH9L C2005 10 04.46068 04 49 13.67 +22 52 40.9 23.0 R EH029675
K03YH9L C2005 10 04.50184 04 49 13.58 +22 52 40.8 22.9 R EH029675
K03YH9L C2005 11 04.48081 04 47 23.87 +22 49 29.2 23 R EH029695
K03YH9L C2005 11 04.51440 04 47 23.71 +22 49 28.8 23 R EH029695
K03YH9M* C2003 12 16.32962 04 47 57.77 +22 45 10.0 24.1 g EH029568
K03YH9M C2003 12 16.35608 04 47 57.62 +22 45 09.7 24.0 g EH029568
K03YH9M C2003 12 16.38238 04 47 57.47 +22 45 09.8 24.1 g EH029568
K03YH9M C2003 12 17.43422 04 47 51.63 +22 45 05.8 EH029568
K03YH9M C2004 12 11.37788 04 53 50.17 +23 29 23.1 24.2 r EH029568
K03YH9M C2004 12 11.40659 04 53 50.01 +23 29 23.0 24.0 r EH029568
K03YH9M C2004 12 11.43951 04 53 49.81 +23 29 22.9 24.1 r EH029568
K03YH9M C2005 11 05.49331 05 02 36.62 +24 13 14.7 EH029695
K03YH9M C2005 11 05.52048 05 02 36.44 +24 13 14.5 EH029695
K03YH9M C2006 01 28.28290 04 55 34.12 +24 10 30.6 EH029675
K03YH9N C2002 11 28.38154 04 54 00.83 +22 59 17.0 EH029568
K03YH9N C2002 11 28.43964 04 54 00.53 +22 59 16.8 EH029568
K03YH9N C2002 11 29.32760 04 53 56.09 +22 59 10.3 EH029568
K03YH9N C2003 10 03.47228 05 02 43.56 +23 14 43.3 23.6 g EH029568
K03YH9N C2003 10 03.52863 05 02 43.48 +23 14 43.4 23.5 g EH029568
K03YH9N C2003 10 03.58452 05 02 43.39 +23 14 43.3 23.1 g EH029568
K03YH9N* C2003 12 16.33292 04 57 51.50 +23 08 54.1 23.7 g EH029568
K03YH9N C2003 12 16.35934 04 57 51.37 +23 08 53.9 23.4 g EH029568
K03YH9N C2003 12 16.38564 04 57 51.23 +23 08 53.5 23.6 g EH029568
K03YH9N C2003 12 17.40463 04 57 46.10 +23 08 46.7 EH029568


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