Kometa C/1999 S4 (LINEAR) Odkrywca LINEAR: Data odkrycia 1999 Elementy orbity: Półoś wielka-7227,9797 au: Mimośród: 1,000106 Peryhelium: 0,7651 au: Nachylenie orbity względem ekliptyki: 149,3851° Długość węzła wstępującego: 83,1808° Argument peryhelium: 151,0503° Moment przejścia przez peryhelium 26 lipca 2000 Charakterystyka

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C/1999 S4 (LINEAR) – Gary W. Kronk Hubble Sees Comet Linear Blow its Top STScI-2000-26 (7. Juli 2000) Comet LINEAR continues to disintegrate and could disappear completely within a few days (31.

214198 214229. S3. 1.8 / 2.0 TFSI. 1999. 2012.

C 1999 s4 linear

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Juli 2000 op eng Distanz vun 0,3724 AE un eis Äerd erun. Den Duerchmiesser vum Koméitekär gouf op ronn 0,9 km geschat. Ier de Koméit sech opgeléist huet, war d'Kärerosiounsquot ongeféier bei 1 cm pro Dag. C/1999 S4 (LINEAR) was a long-period comet discovered on September 27, 1999, by LINEAR. The comet made its closest approach to the Earth on July 22, 2000, at a distance of 0.3724 AU (55,710,000 km; 34,620,000 mi). This is another comet found by the automatic minor planet search program LINEAR in New Mexico.

On the origin of comet C/1999 S4 LINEAR. C. de la Fuente Marcos and R. de la Fuente Marcos. Univ ersidad Complut ense de Madrid, Ciudad Universitaria, 28040 Madrid, Spain. Receiv ed 20 August 2001

DE431 SB-pert. ephem. 2000/7/22 Negative sketch of Comet LINEAR C/1999 S4. 8"/f6 Dob, 25mm eyepiece. The field of view is roughly 1degree.

C 1999 s4 linear

c/1999 s4 (linear) — довгоперіодична комета, відкрита 27 вересня 1999 року в рамках проекту linear. Ближче до Землі комета підійшла 22 липня 2000 року, на відстань 0,3724 a. о. (55 млн км).

140 900 1 00HY024 2000 HYUNDAI Elantra Kombi GLS Aut ABS A/C farth. TOYOTA Yaris 1,0 VVT-i 3d man 99 900 1 00TO002 2000 TOYOTA Yaris 1,0 VVT-i 229 000 1 01AU021 2001 AUDI S4 455 000 1 01AU022 2001 AUDI A4 Avant 2.0t Linear 239 900 1 02SA013 2002 SAAB 9-5 2.3t (185 hk) Linear 254 900 1  B = Saab 9-5 Linear med förar- och passagerarairbag. C #4= Produktlinje A = OG900 B = 99/90. C = 9000. D = NG900/OG9-3.

C 1999 s4 linear

The two-dimensionalcoma morphology indicates a splitting of the nucleus which probably occurred shortlybefore the observations of 28 June 2000. comet C / 1999 S4 LINEAR suggests that it was formed in the inner part of the outer disk of the Solar System, most likely in the Jupiter-S aturn region (Mumma et al. 2001b ) as it w as de- At least 16 fragments were detected in images of comet C/1999 S4 (LINEAR) taken on 5 August 2000 with the Hubble Space Telescope (HST) and on 6 August with the Very Large Telescope (VLT). The evolution of the morphology of C/1999 S4 (LINEAR) is examined from a series of images taken from shortly before the disruption of the nucleus until 10 days afterwards. This is combined with light curve data to provide a unique documentation of the early evolution of the disruption event. A morphological and photometric study of C/1999 S4 (LINEAR) is presented based on data taken with the 1 m Jacobus Kapteyn Telescope (JKT) and 2.5 m Isaac Newton Telescope (INT) at the Observatorio del Roque de los Muchachos and the 82 cm IAC-80 Telescope at Teide Observatory, and visual and CCD data from Spanish amateur astronomers. Here, we present conclusive evidence for detection of x-ray line emission produced by CXE in the first comet observed using the new Chandra X-ray Observatory (CXO).
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C 1999 s4 linear

Comet C/1999 S4 (LINEAR) passed its clos-.

2012. 275507 275511. S4 1.4 TDI / 1.4 TDI Green Line / 1.6 TDI /. 10±3 years, M±SD) observed c/or ’the Outpatient department of Pediatrics Recently, the wave therapy user’impact linear low – tare to Tominaga M, Eguchi H, Manaka H et al (1999) Impairedgastroesophageal reflux, or disease-degenerate-originated in the segments S2-S4 spinal.
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av W Tian · 2019 · Citerat av 73 — We show that CNFs and MXene Ti3C2Tx colloidal dispersions data of FTIR and contact angles (Figure S4, Supporting Information). Ti3C2Tx/CNF nanocomposites with a linear decrease by increasing CNF loading from 5 to 20 wt%. Copyright © 1999-2021 John Wiley & Sons, Inc. All rights reserved.

È stata scoperta il 27 settembre 1999 nell'ambito del programma LINEAR del Lincoln Laboratory (), per la ricerca di asteroidi, quando si trovava a circa 4,33 UA dal Sole, in prossimità dell'orbita di Giove. È stata seguita - salvo una breve parentesi - dal giorno della sua In the current paradigm, Oort cloud comets formed in the giant planets' region of the solar nebula, where temperatures and other conditions varied greatly. The measured compositions of four such comets (Halley, Hyakutake, Hale-Bopp, and Lee) are The results from the analysis of the extensive CCD photometry that we haveobtained during the long-term monitoring (from its discovery until its break-up)of comet C/1999 S4 (linear) are presented here. Our observations showthat the comet did not always behave as expected: it showed activity ahead oftime and in the end became fainter instead of brighter as it approached perihelion.A sequence of 2010-01-01 2007-03-09 Combined BIMA and OVRO Observations of Comet C/1999 S4 (LINEAR) comet C/1999 S4 (LINEAR), hereafter called C/LINEAR, underwent multiple fragmenta-tions during its recent apparition, culminating in the complete disruption of its nucleus during the latter part of July 2000 (5).


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C/1999 S4 Linear. C/1999 S4 Linear 29 images (sum) 20000714 01:41/02:31 UTC Takahashi FS102 ST7. C/1999 S4 Linear (20000714) log scaled C/1999 S4 Linear (20000714) animated GIF (45 min), 01:41/02:31 UTC

av F Jonsson · 2000 · Citerat av 2 — of linear and nonlinear magneto-optical effects are presented in terms of the sus- QELS'99 (Quantum Electronics and Laser Science Conference) Baltimore, USA S4. X a. X b. baS(eemm) ab. (!1 !2 !3 !4). (3.28c).