From "The Origin of Comets by M.E. Bailey, S.V.M. Clube and W.M. Napier, astronomers/astrophysicists.
1
Introduction
"Time and pains will discover what is now unknown and posterity wonder that we did not know such plain things." Seneca.
The problem of the origin of comets is one of the oldest un-solved mysteries in astronomy, with roots pre-dating the ancient Greeks, reaching almost to the dawn of civilization. Comets are also amongst the most primitive astronomical bodies, and the question of their origin is inextricably linked with problems of cosmogony, the formation of stars and the birth of the solar system.
The story of Man's understanding of comets, therefore, is not only associated with the oldest known speculations in natural science and cosmology but also extends to include some of the most recent advances in astrophysics. It makes an excellent backdrop against which to view the development of modern astronomical ideas and concepts, though at times the many interweaving threads of argument may seem rather tangled. In this monograph we attempt to lead the reader through the resulting maze of theory and hypothesis, explaining ideas on comets and their origin from the earliest times right up to the present day.
Advancement of the subject has been closely allied to progress in other fields of astronomy, giving a survey of cometary origins considerable historical interest. Even regarded as a mere instance in the zigzag progression of scientific ideas, the origin of comets soon shows a depth and complexity rarely approached by other individual subjects.
In order to highlight these links with other fields, and to illustrate the apparently perverse back-tracking and retracing of paths that are so often the rule in the progress of science, we have presented the story wherever possible in chronological order. Following this course we hope that the reader may better appreciate the strengths and weaknesses of the arguments about comets which were promoted and believed by leading astronomers and philosophers of the past. The fact that these past arguments have frequently been proved false, or at best only half-true, suggests that the currently accepted picture may even now be largely incomplete.
Although the question of the nature and origin of comets has played an important role in the development of astronomical ideas, the rapid advances made during the present century in new areas of astrophysics — stellar, galactic and extragalactic - have combined almost to overwhelm the traditional disciplines which previously dominated the field. This has been especially true of solar system and cometary astronomy, and it is only in the last decade or so, with the advent of space technology and the launching of vehicles to other planets, that interest in comets and their origin has once again come to the fore.
Indeed, the relative decline of cometary astronomy during this century has been so great that many astronomers nowadays have grown up believing not only that comets are amongst the smallest bodies in the universe but also that they are among the least significant. Popular accounts often seem to mention them only to introduce some disparaging remark about the fear and concern that comets used to arouse among our ancestors, while more serious commentators frequently place them at the end of a book or chapter, seeing them, all too clearly, as merely of secondary interest. Indeed, the problem of the origin of comets is sometimes scarcely mentioned! Given that cosmology and astrophysics are now virtually inseparable, this feeling about the status of comets has inevitably become part of the modern world-view, with an associated tendency to self-perpetuation.
However, the mass of material in comets, setting aside hydrogen and helium, is now believed to be similar to that in stars; but because it is not readily apparent it is not generally reckoned with. Likewise, because the more massive representatives of the cometary flux are not often seen, we tend to ignore both their existence and possible effects on terrestrial evolution. In this way, we may obtain a very distorted image of the importance of comets, including, for example, their potential significance for theories of geological and biological evolution, and for a proper understanding of recorded history. These are weighty issues, and one is bound to ask whether astronomical science has yet produced a balanced view of the origin of comets and their association with the earth.
Indeed, these possible blind spots in modern cometary science have interesting parallels in modern galactic astronomy, where progress is now continually hampered by a lack of knowledge concerning the nature and origin of the unseen 'dark matter'. This too, excusing the pun, is a weighty issue, and it is an interesting speculation whether a solution to all these pressing problems in modern astrophysics will turn out to have major aspects in common. If so, there would be no doubt as to the fundamental importance of cometary studies for cosmology and astrophysics.
For these and many other reasons, not least the arrival of the space age, recent years have seen a resurgence of activity in cometary astronomy. This culminated in 1986, with a rendezvous of Soviet, Japanese and European space probes with Halley's comet. From these we learned, for example, that the activity on the surface of a cometary nucleus is confined to a number of small areas where gas and dust emerge in narrow jets before spreading into the coma and tail (see Figures 1.1 and 1.2). In fact, it seems from the evidence of the jets that comets may be rather porous, low-density bodies, and therefore fragile, whilst their surfaces are more or less asteroidal in appearance. Such findings now provide a firmer foundation on which to base our understanding of how cometary tails are produced and how they evolve under the influence of the solar wind and radiation pressure. But despite these achievements telling us about the appearance and behaviour of observed comets, the question of their origin — whence they come and how they are formed — has proved much harder to resolve.
Nevertheless, this branch of the subject is now also undergoing rapid progress, and important new arguments have recently been advanced which are leading to a complete reappraisal of the previously accepted picture of the nineteen-sixties and seventies. Some of these arguments even hint at a general malaise with the whole concept of a 'primordial' comet cloud, however familiar it may be, suggesting perhaps that the competing idea of an interstellar origin for comets might now have to be taken seriously. An account of these developments is therefore timely, especially considering the part played by Halley's comet in the history of the subject, while this most famous comet is yet fresh in our minds, still influencing the cometary debate worldwide.
1
Introduction
"Time and pains will discover what is now unknown and posterity wonder that we did not know such plain things." Seneca.
The problem of the origin of comets is one of the oldest un-solved mysteries in astronomy, with roots pre-dating the ancient Greeks, reaching almost to the dawn of civilization. Comets are also amongst the most primitive astronomical bodies, and the question of their origin is inextricably linked with problems of cosmogony, the formation of stars and the birth of the solar system.
The story of Man's understanding of comets, therefore, is not only associated with the oldest known speculations in natural science and cosmology but also extends to include some of the most recent advances in astrophysics. It makes an excellent backdrop against which to view the development of modern astronomical ideas and concepts, though at times the many interweaving threads of argument may seem rather tangled. In this monograph we attempt to lead the reader through the resulting maze of theory and hypothesis, explaining ideas on comets and their origin from the earliest times right up to the present day.
Advancement of the subject has been closely allied to progress in other fields of astronomy, giving a survey of cometary origins considerable historical interest. Even regarded as a mere instance in the zigzag progression of scientific ideas, the origin of comets soon shows a depth and complexity rarely approached by other individual subjects.
In order to highlight these links with other fields, and to illustrate the apparently perverse back-tracking and retracing of paths that are so often the rule in the progress of science, we have presented the story wherever possible in chronological order. Following this course we hope that the reader may better appreciate the strengths and weaknesses of the arguments about comets which were promoted and believed by leading astronomers and philosophers of the past. The fact that these past arguments have frequently been proved false, or at best only half-true, suggests that the currently accepted picture may even now be largely incomplete.
Although the question of the nature and origin of comets has played an important role in the development of astronomical ideas, the rapid advances made during the present century in new areas of astrophysics — stellar, galactic and extragalactic - have combined almost to overwhelm the traditional disciplines which previously dominated the field. This has been especially true of solar system and cometary astronomy, and it is only in the last decade or so, with the advent of space technology and the launching of vehicles to other planets, that interest in comets and their origin has once again come to the fore.
Indeed, the relative decline of cometary astronomy during this century has been so great that many astronomers nowadays have grown up believing not only that comets are amongst the smallest bodies in the universe but also that they are among the least significant. Popular accounts often seem to mention them only to introduce some disparaging remark about the fear and concern that comets used to arouse among our ancestors, while more serious commentators frequently place them at the end of a book or chapter, seeing them, all too clearly, as merely of secondary interest. Indeed, the problem of the origin of comets is sometimes scarcely mentioned! Given that cosmology and astrophysics are now virtually inseparable, this feeling about the status of comets has inevitably become part of the modern world-view, with an associated tendency to self-perpetuation.
However, the mass of material in comets, setting aside hydrogen and helium, is now believed to be similar to that in stars; but because it is not readily apparent it is not generally reckoned with. Likewise, because the more massive representatives of the cometary flux are not often seen, we tend to ignore both their existence and possible effects on terrestrial evolution. In this way, we may obtain a very distorted image of the importance of comets, including, for example, their potential significance for theories of geological and biological evolution, and for a proper understanding of recorded history. These are weighty issues, and one is bound to ask whether astronomical science has yet produced a balanced view of the origin of comets and their association with the earth.
Indeed, these possible blind spots in modern cometary science have interesting parallels in modern galactic astronomy, where progress is now continually hampered by a lack of knowledge concerning the nature and origin of the unseen 'dark matter'. This too, excusing the pun, is a weighty issue, and it is an interesting speculation whether a solution to all these pressing problems in modern astrophysics will turn out to have major aspects in common. If so, there would be no doubt as to the fundamental importance of cometary studies for cosmology and astrophysics.
For these and many other reasons, not least the arrival of the space age, recent years have seen a resurgence of activity in cometary astronomy. This culminated in 1986, with a rendezvous of Soviet, Japanese and European space probes with Halley's comet. From these we learned, for example, that the activity on the surface of a cometary nucleus is confined to a number of small areas where gas and dust emerge in narrow jets before spreading into the coma and tail (see Figures 1.1 and 1.2). In fact, it seems from the evidence of the jets that comets may be rather porous, low-density bodies, and therefore fragile, whilst their surfaces are more or less asteroidal in appearance. Such findings now provide a firmer foundation on which to base our understanding of how cometary tails are produced and how they evolve under the influence of the solar wind and radiation pressure. But despite these achievements telling us about the appearance and behaviour of observed comets, the question of their origin — whence they come and how they are formed — has proved much harder to resolve.
Nevertheless, this branch of the subject is now also undergoing rapid progress, and important new arguments have recently been advanced which are leading to a complete reappraisal of the previously accepted picture of the nineteen-sixties and seventies. Some of these arguments even hint at a general malaise with the whole concept of a 'primordial' comet cloud, however familiar it may be, suggesting perhaps that the competing idea of an interstellar origin for comets might now have to be taken seriously. An account of these developments is therefore timely, especially considering the part played by Halley's comet in the history of the subject, while this most famous comet is yet fresh in our minds, still influencing the cometary debate worldwide.