Olaf Stapledon Online

Some utter classics of SF available c/o the Australian Project Gutenberg…

Last and First Men.

…a history of all the human species over the next two aeons. From Earth to Neptune. Written 1930.

Last Men in London.

…a visit by the Neptunian Last Men to our day via mental time-travelling. From 1932.

Star Maker.

…a history of our Cosmos, its Mind, and its ascent towards the Infinite. A glimpse across Eternity. From 1937.

Curiously the stellar physics reflects the change in understanding that astrophysicists had achieved in the 1930s. Prior to nuclear fusion being understood, the stars were believed to potentially be many trillions of years old, slowly burning away their total rest-mass energy. In “Last and First Men” the Sun’s life-span is 10 trillion years, but the planets only appear mid-way through after a James Jeans style near-collision. However by “Star Maker” the lives of the stars were seriously curtailed to mere billions of years and the ‘Big Bang’ provides the cosmic time-scale.

What about prior to Einstein? See my next post…

Iron and Oxygen: A Tale

The Iron Record Of Earth’s Oxygen / Science News.

Oxygen and iron can both exist in aqueous solution, but not together in great quantities. Instead they form insoluble oxides that precipitate out i.e. they make rust! Earth’s oceans haven’t always been as iron poor nor as oxygen rich as they are today. For about 2 billion years – from about 4.4 Gya to 2.3 Gya – they were full of dissolved iron and short on oxygen. As the Science News article, linked to above, reports new research is giving us deeper insights into the “Great Oxygenation Event” of that post-Archean, early Paleo-Proterozoic Era. For example, about 2.316 Gya enough oxygen had built up to form an ozone layer, fundamentally changing the prospects for life ever since.

Geological understanding is built on applying what we know of present day processes to past events – a maxim usually put as “the Present is the Key to the Past”. One present day key-to-the-past is an oxygen-poor lake in Indonesia. Its surface waters are oxygenated, but short on nutrients, then below ~120 metres the water is full of dissolved iron, no oxygen and alive with “photoferrotrophs” – bacteria that use photosynthesis to get energy from oxidising dissolved iron. They live by rusting the iron in the deep lake waters. A feature of the early days of oxygen’s rise are “Banded Iron Formations”, BIFs, from which most of the world’s commercial sources of iron/steel are derived. Basically BIFs are huge rust deposits and the “photoferrotrophs” of the Archean/Paleo-Proterozoic seem to be partially responsible.

What a strange, and humbling, debt we owe to such obscure bacteria. Their metabolic wastes are the ruddy feedstock of the first stage of manufacturing many of modern day industry and construction’s products. The steel skeletons of the Colossii of a modern City come from bacterial chemistry concentrating iron oxides over millennia. And frequently BIFs show a banding effect, now believed to have been caused by seasonal chemistry changes – more rust deposited in warm weather, more silica in cold. But the BIFs keep many more mysteries that geologists have yet to tease out of them…

Brightside of Meteorite bombardment & Junk DNA

Meteorite bombardment may have made Earth more habitable, says study.

Saved by Junk DNA.

The Origin of Life on Earth is a puzzle that biologists, biochemists, physicists and geologists – to name a few – have chewed on over the past 150 years since Darwin opened up the conceptual doors and let in the refreshing light of natural selection. One related question is just when was Earth first inhabited and habitable. The first study above seems to indicate that both Mars and Earth were made more clement by that last gasp of accretion, the Late Heavy Bombardment, which pounded the Inner Planets some 4.0-3.9 billion years ago.

How so? The infalling meteorites released both water and carbon dioxide, thus wetting & warming both planets, perhaps sufficiently for liquid water to remain stable on the open surface. Prior to that event, water may well have been mostly frozen. There’s good reason to think that the process of making long-chains of biomolecules, an important step before ‘Life’ itself, was via concentration of smaller sub-units within ice. Tiny channels of unfrozen liquid become increasingly concentrated in solutes as watery solutions freeze, providing an accelerated reaction environment for polymerisation. In such conditions even quite short pieces of RNA become capable of ‘ligation’, the fusing of RNA sub-units into longer chains.

Once RNA Life has given way to DNA Life what drives the evolution of ever longer strings of DNA and thus ever more complex Life? The second news piece is about evidence that so-called ‘Junk DNA’ – mostly repetitive segments of DNA with no obvious function – actually promotes faster evolution of organisms by altering the rate of gene mutation and gene expression. It seems the ‘Junk’ can make a gene’s DNA sequence more exposed and liable to change when the ‘Junk’ situated next to it has changed in length.

But there’s always a trade off. ‘Junk’ DNA is reduced in some organisms, very noticeably in birds, while it has immensely expanded in some organisms, like certain plants and slow-living creatures like amphibians and lungfish. One’s pace of life style has a distinct selective role on ‘Junk’ DNA’s quantity – fast-living reduces its presence, and perhaps its selective advantage. Birds need to rapidly churn out proteins from their DNA genes and operate at a higher blood temperature too. This might make the DNA more liable to change – birds are immensely speciose – without any ‘Junk’ DNA putting pressure on genes at all. Lungfish, and their kin, live ‘cold-blooded’ rather sedate lives, and carry around a large load of ‘Junk’ that ensures their DNA remains healthy, making the invasion of ‘DNA’ parasites, like viruses, much harder because the host DNA is already full of virus-like ‘Junk’.