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The origin of life from primordial planets

Published online by Cambridge University Press:  22 September 2010

Carl H. Gibson
Affiliation:
University of California San Diego, La Jolla, CA 92093-0411, USA e-mail: cgibson@ucsd.edu
Rudolph E. Schild
Affiliation:
Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA e-mail: rschild@cfa.harvard.edu
N. Chandra Wickramasinghe
Affiliation:
Cardiff Centre for Astrobiology, 24 Llwynypia Road, Lisvane, Cardiff CF14 0SY, UK e-mail: NCWick@gmail.com
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Abstract

The origin of life and the origin of the Universe are among the most important problems of science and they might be inextricably linked. Hydro-gravitational-dynamics cosmology predicts hydrogen–helium gas planets in clumps as the dark matter of galaxies, with millions of planets per star. This unexpected prediction is supported by quasar microlensing of a galaxy and a flood of new data from space telescopes. Supernovae from stellar over-accretion of planets produce the chemicals (C, N, O, P, etc.) and abundant liquid-water domains required for first life and the means for wide scattering of life prototypes. Life originated following the plasma-to-gas transition between 2 and 20 Myr after the big bang, while planetary core oceans were between critical and freezing temperatures, and interchanges of material between planets constituted essentially a cosmological primordial soup. Images from optical, radio and infrared space telescopes suggest life on Earth was neither first nor inevitable.

Information

Type
Research Article
Copyright
Copyright © Cambridge University Press 2010
Figure 0

Fig. 1. Spitzer space telescope infrared view of Helix PNe at 6.7×1018 m. The central white dwarf converts the hydrogen–helium frozen gas of proto-comets shown in the dashed box (bottom insert) to carbon of the shrinking star, and to a plasma jet that partially evaporates the ambient dark matter planets of the PGC clump of dark-matter planets. The red dust cloud about the white dwarf is presumably left by the accreted proto-comets as they evaporate near the star, feeding its growth toward instability.

Figure 1

Fig. 2. Images from the HST of the Helix planetary nebula in the optical (a) and 2.4 μ H2 infrared (b), from Meaburn & Bourmis (2010). Dust from evaporating frozen gas planets at the Oort cavity boundary (b) obscures clumps of merging planets (globulettes, Gahm et al.2007) in the optical (a). Most hydrogen wakes point towards the central white dwarf star ((b), right-hand side). The planet numbered 38 (a) has a 2.4×1014 m diameter atmosphere with mass over 1026 kg, suggesting a massive (~Jupiter) evaporating frozen planet within.

Figure 2

Fig. 3. (a) Images from the Subaru telescope of Helix planets and comets in the 2.4 μ H2 frequency band (i) compared to the HST optical image (ii) in at optical frequencies (Matsuura et al.2009, Fig. 7). Proto-comet planets (i) fall towards the central white dwarf because their biological dust content, atmosphere size and radial radiation pressures are smaller. (b) (i) Shows normalized fluorescence spectra of chloroplasts and phytochrome, which are complex biological PAHs. (ii) ERE first discovered by Witt & Schild (1988) and observed for many galactic and extragalactic sources. (iii) Normalized extinction excess for the gravitationally lensed galaxy SBS0909+522 (at redshift z=0.83) observed by Motta et al. (2002) compared with 115 biological aromatic compounds (see Hoyle & Wickramasinghe 2000). The comparison in (iii) shows that biological waste products were evident in dust when the Universe was half its present size.

Figure 3

Fig. 4. Early formation of gravitational structures supporting life according to HGD. At plasma-to-gas transition the entire baryonic plasma Universe fragments at the gas Schwarz viscous scale LSV to form planets in clumps within proto-clusters and PSCs of proto-galaxies.

Figure 4

Fig. 5. Contrast between HGD and ΛCDMHC timelines for gravitational structures, and for life formation and panspermia. If abiogenesis can work in a time period of a few million years, then all the necessary chemicals, comfortable environments and means of dispersal of the resulting life templates are provided by HGD soon after the plasma-to-gas transition at 1013 seconds. Harsh early conditions of the standard model and its lack of primordial planets make life formation rare and more difficult to disperse.

Figure 5

Fig. 6. Spitzer infrared telescope image of the SMC galaxy at a distance of 70 kpc (~2×1021 m). Dark-matter PGCs with fragmentation scale (M/ρ0)1/3 ~4×1017 m show PAH dust-wake evidence of life occurs only occasionally at PGC scales, and sometimes not at all, as seen for the SMC GC (bottom insert).

Figure 6

Fig. 7. Tadpole galaxy merger brings the BDM halo out of the dark. Nomura-scale galaxy fragments trigger star formation (right insert) in young GCs (YGCs). Tran et al. (2003) identify 42 YGCs, precisely aligned along the star wake path towards frictional mergers of the fragments (Gibson 2008). Schwarz diffusive scales, LSD, are shown for the baryonic and NBDM diffused from the LN-scale proto-galaxy to form BDM and NBDM halos. Background CGCs are fragmented at LN scales along fossil-turbulence vortex lines of the plasma epoch.

Figure 7

Fig. 8. Evidence for big-bang turbulence-driven inflation appears at the smallest wavenumber (largest scale) temperature anisotropies observed by the WMAP fifth microwave background telescope team (a), interpreted here as a fossil of a non-turbulent kinetic energy cascade induced by big-bang turbulent vortices (b).

Figure 8

Fig. 9. Evidence that galaxies form as CGCs along plasma-epoch turbulent vortex lines is provided by Stephan's Quintet. The repaired HST ACS3 and spectrometer (a) make the blue shift of the nearest galaxy obvious, as well as the interpretation (Gibson 2009a, b) that Stephan's Quintet (SQ) is a CGC axial view. Four CGC side views (b) appear in the HST image of the Tadpole galaxy merger.

Figure 9

Fig. 10. Herschel space telescope image from the Eagle star-forming region (box in Fig. 11). Bright infrared objects in the bottom insert are interpreted as large planets and brown dwarf protostars with warm Earth-mass planet wakes evaporated at smaller Oort cavity boundaries than those shown in Fig. 1(a) and (b). The dark PAH-obscured region at the top is interpreted as a PGC clump of strongly life-infected planets, reduced in size and distorted by the strong turbulence of this star-forming region.

Figure 10

Fig. 11. Planck telescope European Space Agency release image from 17 March 2010. Measured temperatures reveal PGC wakes of merged planets triggered into formation by the PGC centre of gravity as it moves through the Milky Way disk, as shown by the arrow. Figure 6 from the dashed box star-forming region shows evidence from PAH dust of turbulent mixing, resulting in the smaller size of the PGCs.

Figure 11

Fig. 12. Herschel space observatory infrared image of the optically dark ‘coalsack’ in the Crux region of the Milky Way disk. PGC scales are shown by dashed circles. Some are dark and some are light. Many are fringed by brightness and show wakes of bright clumps suggesting enhanced PFP planet mergers to form larger planets and gravitationally heated mini-brown-dwarf stars. Darkness and brightness of the PGC clumps is interpreted as PAH evidence of biological activity.

Figure 12

Fig. 13. Microwave background images (Veneziana et al.2010, Figs 1 and 2) from many platforms show redundant images of ‘cirrus dust clouds’ with ‘dust’ temperatures matching frozen hydrogen planet freezing–boiling temperatures TFB=15–20 K. The DIRBE 240 μm image (orange oval) indicates ~106 PGC ‘dust’ clumps similar to the Sgr B2 gmC (right centre). A small molecular cloud in the visible suggests biological dust ejected from evaporated hydrogen planets surrounding an Oort cavity (right top).

Figure 13

Fig. 14. Exclusion diagrams of the MACHO, EROS, and OGLE microlensing collaborations overestimate the number of events to be expected by assuming the MACHO objects (e.g. PFP planets) are not clumped.

Figure 14

Fig. 15. Microbial fossils in comets. (a), (b) Bacterial microfossils in the Murchison meteorite (courtesy of Hans Pflug). (c) A bacterial fossil within a Brownlee particle. (d) a clump of cocci and a bacillus from dust collected using a cryoprobe from 41 km in the atmosphere. References and credits are given in Wickramasinghe et al. (2010).