Antimatter comet

Antimatter comets and antimatter meteoroids are hypothetical comets and meteoroids composed solely of antimatter instead of ordinary matter. Although never actually observed, and unlikely to exist anywhere within the Milky Way, they have been hypothesized to exist, and their existence, on the presumption that hypothesis is correct, has been put forward as one possible explanation for various observed natural phenomena over the years.

Hypothesized existence

The hypothesis of comets made of antimatter can be traced back to the 1940s, when physicist Vladimir Rojansky proposed, in his paper "The Hypothesis of the Existence of Contraterrene Matter", the possibility that some comets and meteoroids could be made from "contraterrene" matter (i.e. antimatter).^[1] Such objects, Rojanski stated, would (if they existed at all) have their origins outside the Solar System.^[2] He hypothesized that if there were an antimatter object in orbit in the Solar System, it would exhibit the behavior of comets observed in the 1940s: As its atoms annihilated with "terrene" matter from other bodies and solar wind, it would generate volatile compounds and undergo a change of composition to elements with lower atomic masses. From this basis he propounded the hypothesis that some objects that had been identified as comets may, in fact, be antimatter objects, suggesting, based upon calculations using the Stefan–Boltzmann law, that it would be possible to determine the existence of such objects within the Solar System by observing their temperatures. An antimatter body subjected to normal levels of meteoric bombardment (per 1940s figures), and absorbing half of the energy created by the annihilation of normal matter and antimatter, would have a temperature of 120 K (−153 °C) for bombardment figures calculated by Wylie or 1,200 K (930 °C) for calculations by Nininger.^[3] In the 1970s, when comet Kohoutek was observed, Rojanski again suggested hypothesis of antimatter comets in a letter in Physical Review Letters, and suggested that gamma-ray observations be made of the comet to test this hypothesis.^[1]^[4]

Rojansky's original 1940 hypothesis was that perhaps the only bodies within the Solar System that could be antimatter were comets and meteoroids, all others being almost certainly normal matter.^[5] Experimental evidence gathered since then has not only borne out this restriction but has made the existence of actual antimatter comets and meteoroids themselves seem ever more unlikely. Gary Steigman, assistant professor of Astronomy at Yale University, observed in 1976 that space probes had proven — by the fact that they were not annihilated upon impact — that bodies such as Mars, Venus, and the Moon were not antimatter. He also noted that had any of the planets or similar bodies been antimatter, their interaction with the terrene solar wind and the sheer strength of the gamma ray emissions that would have resulted^[a] would have made them readily noticeable long since.^[7] He noted that not even antimatter cosmic rays had been found, with all of the nuclei found in studies having been uniformly terrene, the experimental data in several studies made from 1961 onwards by various people excluding the presence of a fractional antimatter composition of cosmic rays any larger than 10⁻⁴ of the total. Further, the uniformly terrene nature of the cosmic ray flux indicates that nowhere in the Milky Way are there any sources of heavier antimatter elements (such as carbon), since (although it is not proven) it is a likely assumption that they represent the overall composition of the entire galaxy. They are representative of the galaxy as a whole — goes the logic — and since they do contain terrene carbon and other atoms, but have not been observed to contain any antimatter atoms, therefore there is no reasonable source for extrasolar antimatter comets, meteoroids, or any other large scale heavy element objects to originate from, within this galaxy.^[8]

Martin Beech from the University of Western Ontario (London, Ontario, Canada) referred to the various hypotheses and experimental results that support non-existence of antimatter in the Universe. He argued that any antimatter comets and meteors that exist must be (at least) extrasolar in origin because the nebular hypothesis for the formation of the Solar System precludes their being solar. Any antimatter in a pre-formation nebula or planetary accretion disc has a comparatively short lifetime, in astronomical terms, before annihilation with the terrene matter that it is mixed with. This lifetime is measured in the hundreds of years, and so any solar antimatter present at the time that the system was formed will have long since been annihilated. Any antimatter comets and meteors must therefore come from another solar system. Furthermore, not only must antimatter meteors be extrasolar in origin, they must have been recently (i.e. within the past 10⁴ ~ 10⁵ years) captured by the Solar System. Most meteoroids are broken down to sizes of 10⁻⁵ g within that timeframe, because of meteoroid-upon-meteoroid collisions. Thus any antimatter meteor must be either extrasolar in origin itself, or broken off from an antimatter comet that is extrasolar in origin. The former are unlikely to exist from observational evidence. Any extrasolar meteoroid would have a hyperbolic orbit, but less than 1% of the observed meteoroids have such, and the process of perturbation of ordinary (terrene) solar objects, by planetary encounters, into hyperbolic trajectories accounts for all of those. Beech concluded that a continued null result, however, does not constitute a proof ('Absence of evidence is not evidence of absence', M. Rees) and a single positive detection negates the arguments presented.^[9]

Hypothesized explanations for observed phenomena

Tektites

In 1947, Mohammad Abdur Rahman Khan, professor at Osmania University and research associate at the Institute of Meteoretics in the University of New Mexico, put forward the hypothesis that antimatter comets or meteoroids were responsible for tektites (Khan 1947). However, this explanation, out of the many proposed explanations for tektites, is considered to be one of the more improbable.^[10]^[11]

Tunguska event of 1908

By the 1950s, speculating about antimatter comets and meteoroids was a commonplace exercise for astrophysicists. One such, Philip J. Wyatt of Florida State University, suggested that the Tunguska event may have been a meteor made of antimatter (Wyatt 1958).^[12] Willard Libby and Clyde Cowan took Wyatt's idea further (Cowan, Atluri & Libby 1965), having studied worldwide levels of carbon-14 in tree rings and noticing unusually high levels for the year 1909. However, even in 1958 the theoretical flaws in the hypothesis were observed, aside from the evidence that was coming in at the same time from the first gamma ray measurement satellites. For one, the hypothesis did not explain how an antimatter meteor could have managed to survive that low into the Earth's atmosphere, without being annihilated as soon as it encountered terrene matter at the upper levels.^[12]^[13]

Ball lightning

In 1971, fragments of antimatter comets or meteoroids were hypothesized, by David E. T. F. Ashby of Culham Laboratory and Colin Whitehead of the U.K. Atomic Energy Research Establishment, as a possible cause for ball lightning (Ashby & Whitehead 1971). They monitored the sky with gamma-ray detection apparatus, and reported unusually high numbers at 511 keV (kilo-electron volts) which is the characteristic gamma ray frequency of a collision between an electron and a positron. There were natural explanations for such readings. In particular positrons can be produced indirectly by the action of a thunderstorm, as it creates the unstable isotopes nitrogen-13 and oxygen-15. However, Ashby and Whitehead noted that there were no thunderstorms present at the times that the gamma-ray readings were observed. They instead presented the hypothesis of antimatter meteors as an interesting one that did explain all of what their observations had recorded, and suggested that it merited further investigation.^[14]^[15]

Gamma-ray bursts

Antimatter comets thought to exist in the Oort cloud were in the 1990s hypothesized as one possible explanation for gamma-ray bursts.^[16] These bursts can be explained by the annihilation of matter and antimatter microcomets. The explosion would create powerful gamma ray bursts and accelerate matter to near light speeds.^[16] These antimatter microcomets are thought to reside at distances of more than 1000 AU.^[16] Calculations have shown that comets of around 1 km in radius would shrink by 1 m if they passed the Sun with a perihelion of 1 AU. Microcomets, due to the stresses of solar heating, shatter and burn up much more quickly because the forces are more concentrated within their small masses. Antimatter microcomets would burn up even more rapidly because the annihilation of solar wind with the surface of the microcomet would produce additional heat.^[16] As more gamma-ray bursts were detected in subsequent years, this theory failed to explain the observed distribution of gamma-ray bursts about host galaxies and detections of X-ray lines associated with gamma-ray bursts. The discovery of a supernova associated with a gamma-ray burst in 2002 provided compelling evidence that massive stars are the origin of gamma-ray bursts.^[17] Since 2002, more supernovae have been observed to be associated with gamma-ray bursts, and massive stars as the origin of gamma-ray bursts has been firmly established.

Footnotes

^ The formula for the predicted gamma ray flux, resulting from annihilation of solar wind particles (taken to be roughly 2×10⁸ cm⁻² sec⁻¹), from a antimatter planet or other Solar System body of radius r at distance d is $F_{gamma}\approx 10^{8}\left({\frac {r}{d}}\right)^{2}$ photons cm⁻² sec⁻¹. This formula predicts a gamma ray flux for the planet Jupiter that is some six orders of magnitude larger than it is actually observed to be. That is, furthermore, without taking into account the fact that other Solar System material in addition to the solar wind infalls to Jupiter.^[6]

References

^ ^a ^b NS 1974a, p. 55
^ Rojansky 1940, p. 258
^ Rojansky 1940, pp. 259–260
^ Rojansky 1973, p. 1591
^ Rojansky 1940, p. 257
^ Steigman 1976, p. 355
^ Steigman 1976, p. 342
^ Steigman 1976, pp. 342–344
^ Beech 1988, p. 215
^ Bagnall 1991, p. 124
^ Vand 1965, p. 57
^ ^a ^b Time 1958
^ Steel 2008
^ NS 1971a, p. 661
^ Charman 1972, p. 634
^ ^a ^b ^c ^d Dermer 1996
^ Bloom et al. 2002, p. L45

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