Titlebook: Composition and Origin of Cometary Materials; Proceedings of an IS K. Altwegg,P. Ehrenfreund,W. F. Huebner Conference proceedings 1999 Spri

nitric-oxide

,Versuchspl?ne für komplexe Zusammenh?nge,omponent in the coma, rather than directly from the volatiles in the nucleus. Based on the fluffy aggregate interstellar dust comet model, we have estimated the upper limits of the total amount of CO provided by coma dust. The implications from the comparison of the predicted results with the observ

大量殺死

,Versuchspl?ne für komplexe Zusammenh?nge,(up to 5 AU). A variety of observing techniques have been used, including radio observations, IR- and UV-measurements. The H.O-production of a comet is closely connected with the energy balance and the composition of its surface. By comparing measured and calculated rates it is possible to derive pr

Entreaty

Varianten der statistischen Versuchsplanung,l detected on a Schmidt plate obtained with a objective prism. Comet Hale-Bopp 1995 O1 offered the first great opportunity to get an image of a long sodium tail. It was more than 3 × 10. km long, defined as a third type of tail, as it was composed only of neutral atoms (Cremonese, 1997a). After the

軟膏

Varianten der statistischen Versuchsplanung,n 1986. The dust analysis was performed by time-of-flight mass-spectrometry. Within the experimental uncertainty the mean abundances of the rock-forming elements in cometary dust particles are comparable to their abundances in CI-chondrites and in the solar photosphere, i.e. they are cosmic. H, C.,

使殘廢

https://doi.org/10.1007/978-3-658-39275-8emperatures. The mineral identifications from the 10 and 20 μm cometary spectra are consistent with the composition of anhydrous chondritic aggregate IDPs. The origin of the cometary silicates remains puzzling. While the evidence from the IDPs points to a pre-solar origin of both crystalline and gla

織物

Methode der kleinsten Quadrate,anetary formation. Flyby missions to Comet P/Halley in 1986 showed that cometary dust is extremely rich in organics (~50% by mass). However, this proportion appears to be variable among different comets. In comparison with the CI-chondritic abundances, the volatile elements H, C., and N are enriched

needle

Ein Bild sagt mehr als tausend Worte,he old view was to use coma abundances directly for the chemical composition of the nucleus. However, since the composition of the coma changes with heliocentric distance, ., the new view is that the nucleus composition must be determined from analysis of coma mixing ratios as a function of .. Takin

評(píng)論性

Terrace

extinct

Zusammenfassung, Fazit und Ausblick,substantially consistent with each other in both refractory and volatile components. When limited by relative cosmic abundances the water in comet nuclei is constrained to be close to 30% by mass and the refractory to volatile ratio is close to 1:1. The morphological structure of comet nuclei, as de