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[Mechanism of radiation death of human peripheral blood lymphocytes, assessed by the DNA-comet method].

Radiation-induced death of human peripheral blood lymphocytes (HPBL) was studied using the comet assay. It has been shown that gamma-irradiation induced simultaneously two forms of death, necrosis and apoptosis which may be discriminated by the comet assay. Three groups of comets formed by HPBL are specified: symmetric/slowly asymmetric comets attributed to viable cells (C0/C1-class of comets); comets reminding "tear-drop" (C3/C4-class of comets) which are characterized by decreased total fluorescence of comet and formed by dying/dead (necrotic or apoptotic) cells; intermediate form of comets (C2-class), containing head, tail and attributed to cells committed to apoptosis (containing high molecular weight fragments of DNA). Kinetics of C2-comets permits detection of early stage of apoptotic death of irradiated HPBL.

Apoptosis↗
PubMed2004

The comet assay as biomarker of heavy metal genotoxicity in earthworms.

The ubiquitous occurring earthworm species, Eisenia fetida, were exposed to nickel chloride to determine whether the heavy metal Ni caused DNA damage, as measured by the comet (single cell gel electrophoresis) assay. Primary cell cultures of earthworm coelomocytes were exposed in vitro and whole animals either in spiked artificial soil water or in spiked cattle manure substrates. Comets formed were scored using mean tail lengths as well as comparing percentages of damage in five different damage classes. The exposure concentrations used for the in vitro exposure (2, 6, and 12 microg/ml) caused the formation of comets of which the mean tail lengths differed significantly (p < 0.05) from those of unexposed controls but not from each other. Coelomocytes from worms exposed in artificial soil water at concentrations of 0.0049, 0.0078, 0.0175, and 0.025 mg/ml formed comets of which the mean tail lengths differed significantly (p < 0.05) between the exposure groups with increasingly longer tail lengths with higher concentration (dose-related response). The tail length means of the comets of the three highest exposure concentrations also differed significantly (p < 0.05) from the controls. No dose-related response was found between comet tail lengths of the three exposure concentrations (60, 240, and 480 mg/kg) used for the worms in the cattle manure substrates, but the mean tail lengths of comets from all three exposure groups differed significantly (p > 0.05) from the controls. The comets formed in cells from animals exposed in artificial soil water and in cattle manure substrates, scored within damage classes, indicated a clear shift with increasing exposure concentrations from low to high damage. Our results indicated DNA single-strand breaks in soil invertebrate cells caused by exposure to a nickel compound, verifying previous findings for mammals which indicated that this heavy metal has genotoxic potential. These results therefore suggest that earthworms may be useful indicator organisms to assess the genotoxic risks of nickel pollution to terrestrial environments and that the comet assay is a useful tool to use as biomarker of genotoxic effects on invertebrates in soil.

Animals↗
PubMed2006

Standard and Fpg-modified comet assay in kidney cells of ochratoxin A- and fumonisin B(1)-treated rats.

The effect of ochratoxin A (OTA), fumonisin B(1) (FB(1)), and their combinations on DNA damage was studied using the standard alkaline comet assay and the Fpg-modified comet assay. Rats were orally receiving OTA (5 ng/kg b.w., 0.05 mg/kg b.w., and 0.5mg/kg b.w., respectively) for 15 days, FB(1) (200 ng/kg b.w., 0.05 mg/kg b.w., and 0.5mg/kg b.w., respectively) for 5 days, and the combinations of two lower OTA and FB(1) doses. The tail length, tail intensity, and Olive tail moment (OTM) obtained with the standard comet assay and Fpg-modified comet assay were significantly higher in treated animals than in controls, even at the lowest dose of OTA or FB(1) (p<0.01). The Fpg-modified comet assay showed significantly greater tail length, tail intensity, and OTM in all treated animal than did the standard comet assay (p<0.05), which suggests that oxidative stress is likely to be responsible for DNA damage. DNA damage detected by the standard comet assay at all OTA or FB(1) doses indicates that some other mechanism is also involved. Combined OTA+FB(1) treatment measured either by the standard comet or the Fpg-modified comet assay showed a synergistic increase in the tail intensity and OTM in kidney cells, even at doses that correspond to the daily human exposure in Europe.

Animals↗
PubMed2003

Comparison of the comet assay and the oxygen microelectrode for measuring tumor oxygenation in head-and-neck cancer patients.

PURPOSE: To compare the Eppendorf PO2 histograph and the alkaline comet assay as methods of measuring tumor hypoxia in patients with head-and-neck squamous cell carcinomas. MATERIALS AND METHODS: As part of a larger clinical trial, 65 patients with head-and-neck squamous cell carcinoma nodal metastasis underwent tumor oxygenation measurements with Eppendorf PO2 histographs and comet assays, performed on fine-needle aspirates at 1 and 2 min after 5 Gy. Fifty-four patients had sufficient tumor cells for comet analysis at 1 min and 26 at both 1 and 2 min. Individual cells were examined for DNA single-strand breaks by alkaline gel electrophoresis, and the distribution of values was quantified using median tail moment (MTM). Nonirradiated tumor cells from pretreatment fine-needle aspirates received 5 Gy in vitro to establish the oxygenated response. RESULTS: There was a significant correlation between the 1- and 2-min MTM (slope = 0.77 +/- 0.03). There was no relationship between DNA damage in tumor cells irradiated in vitro and in vivo. No correlation was found between Eppendorf PO2 measurements and comet MTM. There was a statistically significant correlation between the treatment response in the node studied and comet MTMs, whereas no correlation was observed between treatment response and Eppendorf measurements. CONCLUSIONS: Comet assays are reproducible, as shown by biopsies at 1 and 2 min. Intertumor variation in the MTM is not a result of intrinsic radiosensitivity but of tumor hypoxia. There was no correlation between Eppendorf PO2 measurements and comet MTM. Comet assays were better than Eppendorf in predicting treatment response as an end point for short-term outcome. Longer follow-up is needed to determine the role of the comet assay as a predictor for locoregional tumor control and survivals.

Adult↗
PubMed2000

Comet assay: rapid processing of multiple samples.

The present study describes modifications to the basic comet protocol that increase productivity and efficiency without sacrificing assay reliability. A simple technique is described for rapidly preparing up to 96 comet assay samples simultaneously. The sample preparation technique allows thin layers of agarose-embedded cells to be prepared in multiple wells attached to a flexible film of Gelbond, which improves the ease of manipulating and processing samples. To evaluate the effect of these modifications on assay sensitivity, dose-response curves are presented for DNA damage induced by exposure of TK6 cells to low concentrations of hydrogen peroxide (0-10 microM) and for exposure of human lymphocytes to X-irradiation (0-100 cGy). The limit of detection of DNA damage induced by hydrogen peroxide in TK6 cells was observed to be 1 uM for all parameters (tail ratio, tail moment, tail length and comet length) while the limit of detection of DNA damage in human lymphocytes was 10 cGy for tail and comet length parameters, but 50 cGy for tail ratio and tail moment parameters. These results are similar to those previously reported using the conventional alkaline comet assay. The application of SYBR Gold for detection of DNA damage was compared to that of propidium iodide. Measurements of matching samples for tail length and comet length were similar using both stains. However, comets stained with SYBR Gold persisted longer and were much brighter than those obtained with propidium iodide. SYBR Gold was found to be ideal for measuring tail length and comet length but, under present assay conditions, impractical for measuring tail ratio or tail moment due to saturation of staining in the head region of the comets.

Cell Line↗
PubMed2005

DNA damage induced by a quinoxaline 1,4-di-N-oxide derivative (hypoxic selective agent) in Caco-2 cells evaluated by the comet assay.

The DNA damage induced by 7-chloro-3-[[(N,N-dimethylamino)propyl]amino]-2-quinoxalinecarbonitrile 1,4-di-N-oxide hydrochloride (Q-85 HCl) in Caco-2 cells under hypoxic and well-oxygenated conditions has been studied by using the comet assay. This compound has shown a good in vitro profile of high selective toxicity in hypoxia, but its mechanism of action is unknown. The DNA damage has been evaluated by performing the comet assay after a 2-h treatment with Q-85 HCl (0.1, 0.2, 0.4 microM in hypoxia; 20, 40 microM in well-oxygenated conditions). The number of cells in apoptosis has also been assessed by flow cytometry analysis of Annexin V-FITC staining. The capability of the cells to repair the DNA damage and the proliferation rate was evaluated at different times after the treatment (24-168 h). Under hypoxic conditions, a clear dose-dependent increase in the number of nuclei with a comet was observed (comet score: 132 +/- 13, 343 +/- 30 and 399 +/- 1; control comet score: 42 +/- 14). Under well-oxygenated conditions, the number of nuclei with comet increased significantly with respect to the control (comet score: 273 +/- 14 and 312 +/- 9; control comet score: 27 +/- 4). Cells in apoptosis were not detected by the comet assay nor by flow cytometry. The recovery from DNA damage was time- and concentration-dependent in hypoxia (cells treated with the highest concentration still showed DNA damage after 72 h) and rather time-dependent in well-oxygenated conditions (DNA was completely repaired after 24 h). In conclusion, Q-85 HCl acts by DNA damage and not only the reduced intermediate is genotoxic but also some other derivatives and Q-85 HCl itself may be acting.

Apoptosis↗
PubMed2002

The large GTPase dynamin regulates actin comet formation and movement in living cells.

The large GTPase dynamin (Dyn2) has been demonstrated by us and others to interact with several different actin-binding proteins. To define how Dyn2 might participate in actin dynamics in livings cells we have expressed green fluorescent protein (GFP)-tagged Dyn2 in cultured cells and observed labeling of comet-like vesicles and macropinosomes. The comet structures progressed with a constant velocity and were reminiscent of actin comets associated with motile vesicles in cells expressing type I phosphatidylinositol phosphate 5-kinases. Based on these observations we sought to determine whether Dyn2 is an integral component of actin comets. Cells expressing type I phosphatidylinositol phosphate 5-kinase and Dyn2-GFP revealed a prominent colocalization of Dyn2 and actin in comet structures. Interestingly, comet formation and motility were normal in cells expressing wild-type Dyn2-GFP but altered markedly in Dyn2 mutant-expressing cells. Dyn2K44A-GFP mutant cells displayed a significant reduction in comet number, length, velocity, and efficiency of movement. In contrast, comets in cells expressing Dyn2DeltaPRD-GFP appeared dark and did not incorporate the mutant Dyn2 protein, indicating that the proline-rich domain (PRD) is required for Dyn2 recruitment. Further, these comets were significantly longer and slower than those in control cells. These findings demonstrate a role for Dyn2 in actin-based vesicle motility.

Actins↗
PubMed2000

The use of silver-stained "comets" to visualize DNA damage and repair in normal and Xeroderma pigmentosum fibroblasts after exposure to simulated solar radiation.

The alkaline and neutral comet assays have been widely used to assess DNA damage and repair in individual cells after in vivo or in vitro exposure to chemical or physical genotoxins. Cells processed under neutral conditions generate comets primarily from DNA double strand breaks, whereas under alkaline conditions, comets arise from DNA single and double strand breaks and alkali-labile lesions. A modified version of the alkaline comet assay, as described here, used silver stain to visualize the comets and a Gelbond base to facilitate the manipulation and processing of samples. To demonstrate how these modifications improve the assay, fibroblasts derived from both normal and Xeroderma pigmentosum (Xp) individuals were exposed to simulated solar radiation and the resulting DNA damage and repair evaluated and compared with results from the relevant literature. Comets from normal fibroblasts reached their maximum length at about an hour after irradiation. Dose-dependent increases in comet length were observed up to at least 360 mJ/cm2. In contrast, comet lengths from repair deficient Xp fibroblasts were shorter than normal cells reflecting their reduced capacity to generate single strand breaks by the excision of DNA dimers. For incubation times of more than 1 h, comet lengths from normal fibroblasts underwent a time-dependent decrease, supporting the contention that this change was related to the ligation step in the DNA repair process. These changes were compatible with the model of DNA damage and repair established by others for ultraviolet radiation.

Cell Line↗
PubMed1989

Infrared emission from comets.

A brief discussion of the infrared observations from 4 to 20 micrometers of seven comets is presented. The observed infrared emission from comets depends primarily on their heliocentric distance. A model based on grain populations composed of a mixture of silicate and amorphous carbon particles in the mass ratio of about 40 to 1, with a power-law size distribution similar to that inferred for comet Halley, is applied to the observations. The model provides a good match to the observed heliocentric variation of both the 10 micrometers feature and the overall thermal emission from comets West and Halley. Matches to the observations of comet IRAS-Araki-Alcock and the antitail of comet Kohoutek require slightly larger grains. While the model does not match the exact profile and position of the 3.4 micrometers feature discovered in comet Halley, it does produce a qualitative fit to the observed variation of the feature's strength as a function of heliocentric distance. The calculations predict that the continuum under the 3.4 micrometers feature is due primarily to thermal emission from the comet dust when the comet is close to the Sun and to scattered solar radiation at large heliocentric distances, as is observed. A brief discussion of the determination of cometary grain temperatures from the observed infrared emission is presented. It is found that the observed shape of the emission curve from about 4 to 8 micrometers provides the best spectral region for estimating the cometary grain temperature distribution.

Astronomical Phenomena↗
PubMed2005

Comparative evaluation of the alkaline comet assay with the micronucleus test for genotoxicity monitoring using aquatic organisms.

A comparative analysis between the in vivo comet assay and the in vivo micronucleus test (MNT) was carried out in three aquatic organisms suitable for genotoxicity monitoring, carp (Cyprinus carpio), rainbow trout (Oncorhynchus mykiss), and clam (Spisula sachalinensis), using a direct-acting mutagen, N-methyl-N'-nitro-N-nitrosoguanidine (MNNG), and an indirect mutagen, benzo[a]pyrene (B[a]P). By optimizing the conditions for cell isolation, gill and liver (or digestive glands) were selected as test tissues of the comet assay for MNNG and B[a]P. The MNT employed the erythrocytes (or hemocytes), the most universal cell type for the assay. The analysis of DNA strand breaks using the comet assay and the micronucleus frequencies using the MNT revealed dose- and time-dependent increases between animals exposed to several concentrations of mutagens. But the statistical significance (P<0.05) obtained was higher by the comet assay than by the MNT. When the time profiles of genotoxic signals resulting from B[a]P exposure to carp were plotted representatively, clear distinctions between all concentrations were made in the comet assay, but not in the MNT. The correlation index defined in this study also showed a higher correlation between concentration and signal in the comet assay than in the MNT. It is suggested that the standardization of the comet assay is necessary for its methodological evaluation and use as a genotoxicity biomarker. We conclude that the comet assay has an excellent suitability for aquatic genotoxicity monitoring because of its high and reliable sensitivity.

Animals↗
PubMed2004

Relationship between human semen parameters and deoxyribonucleic acid damage assessed by the neutral comet assay.

OBJECTIVE: To explore the association between semen parameters and sperm DNA damage. DESIGN: Cross-sectional. SETTING: Andrology clinic. PATIENT(S): Two hundred fifty-seven men undergoing infertility assessment. INTERVENTION(S): None. MAIN OUTCOME MEASURE(S): Sperm concentration and motility were measured using computer-assisted sperm analysis; morphology was scored using the strict criteria. The neutral comet assay was used to measure sperm DNA damage. Comet assay parameters included comet extent, percent DNA in the comet tail, and tail distributed moment, an integrated measure of length and intensity. We also scored cells that were too long to measure (>300 microm), which we referred to as cells with high DNA damage. RESULT(S): Men older than 35 years had a statistically significant increase in the number of cells with high DNA damage as compared with younger men. In age-adjusted regression analyses, the most consistent associations were found between semen parameters and the number of cells with high DNA damage. For an interquartile range change in the number of cells with high DNA damage, sperm concentration declined 14.2 x 10(6)/mL, motility declined 4.3%, and morphology declined 0.5%. Comet extent and percent DNA in the comet tail were also associated with a decline in sperm concentration and motility, respectively. CONCLUSION(S): Although there were associations between semen and comet assay parameters, their magnitudes were weak, suggesting that the comet assay provides additional independent information on sperm function.

Adult↗
PubMed2007

Measurements of DNA damage on silver stained comets using free Internet software.

Silver stain offers the possibility to stain comets permanently, but up to now it was impossible to measure the majority of the comet parameters, because the distinction between head and tail was not recognised by software. Here, we report a silver staining protocol that allows the measurement of comet parameters using the free Internet software CASP. We validated the silver stain protocol by comparing the behaviour of the parameter '% DNA in tail' in silver and fluorescent stained comets. The range of % DNA in tail for different visual categories of damage in silver stained comets was similar to that reported with fluorescence staining. The range was for category 0 (no damage), <1%; category 1 (low damage), 1-25%; category 2 (medium damage), >25-45%; category 3 (high damage), >45-70%; category 4 (very high damage), >70%. The mean of % DNA in tail in silver stained comets was also similar to that reported with fluorescence staining. The mean was for category 0, 0.4+/-0.34%; category 1, 12+/-7%; category 2, 37+/-4%; category 3, 57+/-5% and category 4, 83+/-6%. Others comet parameters such as tail length, tail moment and Olive tail moment can be also measured. The silver staining protocol reported here opens new opportunities for those working in the assay without fluorescent microscope as the measurement of comet parameters using free Internet software and conventional microscope becomes possible.

Comet Assay↗
PubMed2003

Comparison of comet assay, electron microscopy, and flow cytometry for detection of apoptosis.

Differentiating apoptosis from necrosis is a challenge in single cells and in parenchymal tissues. The techniques available, including in situ TUNEL (Terminal deoxyribonucleotide transferase-mediated dUTP-X Nick End-Labeling) staining, DNA ladder assay, and flow cytometry, suffer from low sensitivity or from a high false-positive rate. This study, using a Jurkat cell model, initially evaluated the specificity of the neutral comet assay and flow cytometry compared to the gold standard, electron microscopy, for detection of apoptosis and necrosis. Neutral comet assay distinguished apoptosis from necrosis in Jurkat cells, as evidenced by the increased comet score in apoptotic cells and the almost zero comet score in necrotic cells. These findings were consistent with those of electron microscopy and flow cytometry. Furthermore, using rats with burn or ischemia/reperfusion injury, well-established models of skeletal and cardiac muscle tissue apoptosis, respectively, we applied the comet assay to detect apoptosis in these muscles. Neutral comet assay was able to detect apoptotic changes in both models. In the muscle samples from rats with burn or ischemia-reperfusion injury, the comet score was higher than that of muscle samples from their respective controls. These studies confirm the consistency of the comet assay for detection of apoptosis in single cells and provide evidence for its applicability as an additional method to detect apoptosis in parenchymal cells.

Animals↗
PubMed2005

The comet-FISH technique: a tool for detection of specific DNA damage and repair.

The comet-FISH technique described in this protocol is a tool to detect genome region-specific DNA damage and repair. It is a combination of two established techniques, the comet assay (or single-cell gel electrophoresis, or the single-cell gel test), to separate highly fragmented from moderately or nonfragmented DNA and to measure it, and fluorescence in situ hybridization (FISH), to specifically label DNA sequences of interest. Comet-FISH exists in two versions, based on the neutral and the alkaline comet assays. A detailed description of the comet assay is given in Chapter 9, so readers who are not familiar with this technique can work directly with the protocol described here, without referring to additional protocols reported elsewhere. The neutral version of the comet assay detects double-strand breaks, while the alkaline version detects both double- and single-strand breaks as well as abasic sites or sites of incomplete repair. This chapter also details cell preparation and production of the hybridization probes adapted to the comet-FISH technique. Finally, microscopic analysis of comet-FISH results is described, and possible procedures of quantification of the specific DNA damage are presented.

Animals↗
PubMed2000

Measurement of hypoxia using the comet assay correlates with preirradiation microelectrode pO2 histography in R3327-AT rodent tumors.

Polarographic determination of tumor oxygenation by Eppendorf histography is currently under investigation as a possible predictor of radiotherapy outcome. Alternatively, the alkaline comet assay has been proposed as a radiobiological approach for the detection of hypoxia in clinical tumor samples. Direct comparisons of these methods are scarce. One earlier study with different murine tumors could not establish a correlation, whereas a weak correlation was reported for a variety of human tumors. Considering the different end points and spatial resolution of the two methods, a direct comparison for a single tumor entity appeared desirable. Anaplastic R3327-AT Dunning prostate tumors were grown on Copenhagen rats to volumes of 1-6 cm(3). Eppendorf histography (100-200 readings in 5 parallel tracks) for 8 different tumors revealed various degrees of oxygenation, with median pO(2) values ranging from 1.1 to 23 mmHg. Within 5 min after an acute exposure to 8 Gy (60)Co gamma rays, tumors were excised from killed animals and rapidly cooled to limit repair, and a single cell suspension was prepared for use with the comet assay. The resulting comet moment distributions did not exhibit two subpopulations (one hypoxic and the other aerobic), and a hypoxic fraction could not be calculated. Instead, the average comet moment distribution was taken as a parameter of overall strand break induction. Corresponding experiments with tumor cells grown in vitro allowed us to derive the relationship between the oxygen enhancement ratio (OER) for the average comet moment and oxygen partial pressure (Howard-Flanders and Alper formula). The validity of this relationship was inferred for cells exposed in situ, and the convolution of a pO(2) distribution with the formula of Howard-Flanders and Alper yielded an array of expected OER values for each tumor. The average expected OER correlated well with the average comet moment (r = 0.89, P < 0.01), and the in situ comet moment distributions could be predicted from the Eppendorf data when 50% repair was taken into account, assuming a 5-min damage half-life. The findings confirm the potential of interstitial polarography to reflect radiobiologically relevant intracellular oxygenation, but also underscore the confounding influence of differences in repair that may occur when cells are prepared from irradiated tissues for use with the comet assay.

Adenocarcinoma↗
PubMed1996

Substantial outgassing of CO from comet Hale-Bopp at large heliocentric distance.

When comet C/1995 O1 (Hale-Boop) was discovered, at a distance of seven astronomical units from the sun, it was more than one hundred times brighter than comet Halley at the same distance. A comet's brightness is derived from the reflection of sunlight from dust grains driven away from the nucleus by the sublimation of volatile ices. Near the sun, sublimation of water ice (a main constituent of comet nuclei) is the source of cometary activity; but at its current heliocentric distance, Hale-Boop is too cold for this process to operate. Other comets have shown activity at large distances, and in the case of comet Schwassmann-Wachmann 1, carbon monoxide has been detected in quantities sufficient to generate its observed coma. Here we report the detection of CO emission from Hale-Boop, at levels indicating a very large rate of outgassing. Several other volatile species were searched for, but not detected. Sublimation of CO therefore appears to be responsible for the present activity of this comet, and we anticipate that future observations will reveal the onset of sublimation of other volatile species as the comet continues its present journey towards the sun.

Carbon Monoxide↗
PubMed1989

Chemical evolution of interstellar dust, comets and the origins of life.

It now appears that the chemical evolution of the pre-solar system interstellar dust ensures that a major fraction of comets is in the form of complex organic molecules at least partially of a prebiotic nature and that the submicron interstellar dust preserves its chemical integrity as result of forming a very tenuous low density comet structure whose solid matter occupies approximately 1/5 of the total volume. This low density micro structure further provides a physical basis for comets bringing a significant fraction of the original interstellar organic molecules to the earth unmodified by the impact event. Finally, the evidence for a large number of comet collisions with the early earth ensured that the major organic molecular budget on the earth's surface was "continuously" supplied along with water well before 3.8 billion years ago which is the earliest date for life. The chemistry and morphological structure of a comet nucleus as an aggregate of interstellar dust is used to provide comparisons with a variety of comet Halley results: the density of the nucleus and of the dust; the dust cloud model and its consequences on the production of C+ and CN in the coma by small organic grains; the surface albedo and the low nucleus heat conductivity and high surface temperature; the appearance of 10(-14) g and 10(-17) g dust particles along with higher masses; the mass spectra of dust and infrared spectroscopy as evidence for complex organic grain mantles and of very small (approximately 0.01 micrometer) carbonaceous and silicate grains; the appearance of small grains resulting from breakup of larger grains. The cosmic ray dosage of a comet nucleus during its 4.5 billion years in the Oort cloud appears to be many orders of magnitude less than the dosage of the preaggregated interstellar dust by ultraviolet photons except perhaps in the outer few meters of the nucleus of a new comet. The heat conductivity calculated for aggregated dust is certainly less than 10(-4) that of crystalline ice. This, in combination with the interstellar dust microstructure, provide a basis for showing that solar heating of the interior of a nucleus is lower than previously estimated.

Carbon↗
PubMed2001

Constraints on nebular dynamics and chemistry based on observations of annealed magnesium silicate grains in comets and in disks surrounding Herbig Ae/Be stars.

Understanding dynamic conditions in the Solar Nebula is the key to prediction of the material to be found in comets. We suggest that a dynamic, large-scale circulation pattern brings processed dust and gas from the inner nebula back out into the region of cometesimal formation-extending possibly hundreds of astronomical units (AU) from the sun-and that the composition of comets is determined by a chemical reaction network closely coupled to the dynamic transport of dust and gas in the system. This scenario is supported by laboratory studies of Mg silicates and the astronomical data for comets and for protoplanetary disks associated with young stars, which demonstrate that annealing of nebular silicates must occur in conjunction with a large-scale circulation. Mass recycling of dust should have a significant effect on the chemical kinetics of the outer nebula by introducing reduced, gas-phase species produced in the higher temperature and pressure environment of the inner nebula, along with freshly processed grains with "clean" catalytic surfaces to the region of cometesimal formation. Because comets probably form throughout the lifetime of the Solar Nebula and processed (crystalline) grains are not immediately available for incorporation into the first generation of comets, an increasing fraction of dust incorporated into a growing comet should be crystalline olivine and this fraction can serve as a crude chronometer of the relative ages of comets. The formation and evolution of key organic and biogenic molecules in comets are potentially of great consequence to astrobiology.

Journal Article↗