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Journal ArticleDOI

The organic nature of cometary grains

TLDR
In this article, a model with varying contributions from bacterial-type and viral-type particles, and with small additional contributions arising from degraded organic molecules at grain surfaces, is presented.
Abstract
Infrared observations of comets over the 2–4 Μm waveband are interpreted in terms of a model with varying contributions from bacterial-type and viral-type particles, and with small additional contributions arising from degraded organic molecules at grain surfaces.

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Citations
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Journal ArticleDOI

Influenza--evidence against contagion: discussion paper.

TL;DR: At the end of the last century most medical practitioners took it for granted that influenza could not be fully reconciled with the idea of contagion alone, and person-toperson spread was considered an unlikely mechanism to operate over relatively large geographical areas.
Journal ArticleDOI

Significant broadband extinction abilities of bioaerosols

TL;DR: In this article, the authors measured the reflectance spectra of 12 common biomaterials and calculated their complex refractive indexes at wavelengths of approximately 0.7, 2.1, 6.1 and 9.5μm.
Journal ArticleDOI

Cometary habitats for primitive life.

TL;DR: Subsurface lakes on the Europa model, though insulated by some metres of ice, would require a trigger (perhaps meteorite impact and energy source) to initiate and maintain a suitable-habitat on short period comets.
Book ChapterDOI

Elevating the Status of Dust

TL;DR: The subject of interstellar grains has grown enormously in stature over the past 40 years, the duration of my collaboration with Fred Hoyle as mentioned in this paper, in large measure due to Fred's prescient inputs into this subject and his encouragement.
Journal ArticleDOI

Cometary organics and the 3.4μm spectral feature

TL;DR: The 3.4μm feature corresponds to stretching vibrations of the C-H bond, with details over 3.3-3.5μm depending on neigbouring molecular bonds as mentioned in this paper.
References
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Journal ArticleDOI

The organic component in dust from comet Halley as measured by the PUMA mass spectrometer on board Vega 1

TL;DR: In this paper, the composition of cometary dust has been analyzed by mass spectroscopy, showing that most particles consist of a predominantly chondritic core with an organic mantle composed mainly of highly unsaturated compounds.
Journal ArticleDOI

Composition of comet Halley dust particles from Giotto observations

TL;DR: The mass spectra of cometary dust particles measured by the PIA dust particle analyzer aboard the Giotto spacecraft showed some unexpected and striking features as mentioned in this paper, such as small particles below 10 to the -14th g are much more abundant than anticipated by models.
Journal ArticleDOI

Discovery of organic grains in comet Halley

TL;DR: In this paper, a broad absorption band at a central wavelength of 3.4 μm along the line of sight to IRS7, a luminous star near the galactic centre, was detected in the spectrum of the comet Halley.
Journal ArticleDOI

Diffuse interstellar absorption bands between 2.9 and 4.0 µm

D. A. Allen, +1 more
- 01 Nov 1981 - 
TL;DR: In this paper, a broad absorption trough with numerous discrete features stretching from 2.9 to 3.6 µm was found, indicating that complex organic molecules may be involved in the absorption process.

Diversity and similarity of comets

TL;DR: The evolution of comets from an early stage where they were all similar, to the later diversity is reviewed in this article, where the elemental abundances of pristine comets are likely to be primitive, that is in solar abundance ratios for all elements including C, N, O, S, but with the exception of H (and assumedly He and Ne) that are severely depleted.
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