stable disequilibria, catalytic metabolisms, periodic physiological
cycles, and homeostatic feedback controls qualify stars as living
physicist and science writer John Gribbin argues on behalf of "the
living universe." The phrase is meant to capture similarities
between cosmic and biological processes. If the Earth’s biosphere
can be considered a discrete living unity—the
so too can the Milky Way, or any other spiral galaxy, Gribbin
argues. Like Gaia, a spiral galaxy maintains itself in a state
of stable disequilibrium through the use of feedback controls. Like an organism, it manages its internal physical
processes in the way needed to maintain its characteristic form.
Spiral galaxies in this way exhibit a managed degree of homeostasis—an essential
characteristic of living organisms.
as eager as Gribbin is to classify the Milky Way as an organism, he is
less generous when it comes to individual stars. As dynamic and lively
as they are in terms of their internal processes, stars don't make the cut. "The life processes that
create and maintain the spiral structure in disk galaxies start with stars,"
Gribbin acknowledges, and he concedes that stars possess a trait distinctive
of living things: "A star like our sun is itself, of course, in a
state far from equilibrium." But we should not be misled by that
fact: "Not even the keenest enthusiast for the Gaia hypothesis would
argue that the sun is alive in the way that the Earth and the Milky Way
are alive, because the sun is doing the best it can to reach equilibrium."
"The most useful tool astronomers have for studying the way
stars change as they age is called the Hertzsprung-Russell diagram, after
the two astronomers who pioneered its use. Stars live for so long and change
so slowly, by and large, that there is no hope of studying stellar evolution
by watching an individual star or two age. But the H-R diagram enables
astronomers to do the equivalent of a botanist who studies a forest of
trees that includes seedlings, saplings, and mature specimens and uses
those studies to work out the life cycle of a tree."
dismissiveness reveals a bias.
The sun might be succumbing to entropy—rolling
down the slope of potential energy toward equilibrium—despite its
best efforts, just as are all of us who find ourselves past mid life. But one would not likely characterize a healthy, growing child as "doing the best it can to reach equilibrium." Why would one characterize a healthy, growing young star that way? The suitability of the characterization—heading toward equilibrium—depends on life-cycle stage, not on the particular organism, biological or stellar, under consideration.
Stars embody such a striking number of organismic traits
that a reclassificication is called for. The star larvae
hypothesis extends the notion of being alive specifically and explicitly
to stars. And if stardom pulls history into the future, then humans have some responsibility to facilitate the program. The star larvae hypothesis situates not only natural history in the context of stellar ontogeny, but pulls along human history as well. We might not be the captains of our fate that we like to imagine ourselves to be. Human history is as much an unfolding of natural processes as is evolutionary history, or the early stages of stellar ontogeny.
The stellar organism exhibits the following traits.
Stars maintain themselves by releasing
nuclear energy from the smaller atomic nuclei that they fuse into larger nuclei. Animals maintain
themselves by releasing chemical energy
from the foods they eat to produce the chemical constituents of their bodies. Plants exploit freely available solar energy to produce the bodily constituents that they need. Like biological metabolism, a stellar metabolism uses energies released by its internal processes to maintain itself in a state of stable disequilibrium.
consists of interwoven processes of nuclear fusion and fission that maintain the gross structures and processes
of the star's anatomy and physiology. These processes correspond to the anabolic (building up) and catabolic (tearing down) processes, respectively, that compose biological metabolism. Newborn stars consume hydrogen nuclei
(unattached protons), exclusively. The processes that fuse these protons
into the nuclei of larger atoms occur by various, specific nuclear reactions.
Inside stars, reactions, such as the proton-proton
chain, the triple
alpha process, and the CNO
cycle, build up larger atomic nuclei from individual
protons. The term for this process is nucleosynthesis.
The prevalence among the above listed and other reaction pathways, relative to one another, varies with the
age of a star, a situation that parallels metabolic changes that occur
in aging biological organisms. A newborn star fuses individual protons (hydrogen nuclei)
into proton pairs (helium nuclei) during the star's hydrogen
burning stage. Eventually
too few free protons remain to keep the process going, but sufficient
numbers of helium nuclei have been created for the star to shift into
a hotter, helium-burning phase. This nucleosynthetic process fuses helium
nuclei into carbon, nitrogen, oxygen and other larger atoms. Eventually
a star will burn carbon and larger atoms and fuse them into yet larger ones,
with iron defining the upper size limit of atoms that are formed through
the metabolic processes that dominate the life of a typical star. Shorter-lived
but more energetic processes produce the atoms that are heavier
than iron. These processes take place during the explosive, high-energy
events that constitute the death throes of a star.
a star bigger than the sun, a peculiarity during the hydrogen
burning phase underscores a shared behavior of stars and biological organisms. If the particle cloud that gives birth to a star
contains enough carbon, nitrogen, and oxygen, then the star will initiate a
mode of hydrogen burning called the CNO cycle, in which it fuses hydrogen
nuclei into helium nuclei through a catalytic process. Catalysis is a
transformative process that relies on intermediaries that participate in reactions
but emerge unchanged once the reactive cycle completes. Enzymes provide an example from biology. Certain enzymes will bond to particular molecules, introduce those molecules
to others, then detach themselves from the molecules that they have joined together. Catalytic enzymes emerge unchanged by the reactions that they catalyze.
the catalytic CNO cycle, isotopes of carbon, nitrogen, and oxygen exchange
protons, and emit subatomic particles through radioactive decay, in a specific
sequence of transformations that yields helium from an initial union
of hydrogen and carbon. Each time a helium nucleus is emitted from the
process it leaves behind the original carbon isotope, which is then free
to bond with another hydrogen nucleus—proton—and begin
the cycle again. The process is a true catalysis. When the manufactured
helium is released, the initiator of the process is regenerated and begins
the cycle again.
Notice the elements involved in this catalytic process: carbon, hydrogen, oxygen and nitrogen. This group of elements, sometimes
designated by the abbreviation CHON, constitutes up to 90 percent of the
mass of biological protoplasm. Surely it is s a strange coincidence that
these elements also play starring roles in the catalytic metabolisms of stars. No reason exists, a priori, to expect that the nuclear and chemical properties of these elements would dovetail so neatly. The star larvae hypothesis sees in the coincidence evidence of familial descent.
Anatomy and Physiology
In addition to exploiting catalysis, stars exhibit a list of attributes readily couched in biological language. A star comprises internal arrangements of stable yet dynamically interacting
subsystems that constitute its anatomy. The
material and energetic exchanges within and among the subsystems constitute the
Despite appearances, a star is an organized structure of discernible
components arranged and interacting with one another in definite ways.
not a homogeneous blob of hot gas. The anatomy of our sun, for example, comprises, an inner core
within which nucleosynthesis occurs, a radiative layer that carries energy
out from the core by radiation, and a convective layer that carries the
energy further by convection. This onion-like structure continues outward
from the core to the periphery, through the photosphere, the chromosphere,
and, at the outer fringes, the diffuse corona.
body plan is maintained physiologically.
The photosphere, for example, includes structures that solar physicists
call granules, which are the tops of convection cells that cover
the sun. The convection cells underlying the granules constitute a circulatory
system that shuttles material between the interior and the surface of
the solar body. At the surface the fluid material circulates according
to multiple flow components (rotation, cellular convection, oscillations,
and meridional flows).The granules themselves compose supergranules,
whose fluid motions concentrate magnetic fields to produce a weblike
pattern of field lines—the chromospheric network—that continually
evolves over the sun’s surface. The photospheric circulatory system
includes magnetic field markers—the familiar sunspots—and
the smaller, brighter spots called faculae. A system of interlocking
processes is at work here to maintain a discernible, complex structure
in a state of stable disequilibrium and which exhibits a level of complexity highly
suggestive of a living organism.
other organisms, a star's internal processes are cyclic. In biological organisms, cyclic processes include the familiar circadian, ultradian and infradian
rhythms of animals, such as sleep/wake, respiratory and estrus cycles. Gaia, too, pulses rhythmically, with tidal, seasonal, glacial, and other cycles. The sun exhibits the same tendency.
Its rhythms include the well-studied eleven-year
sunspot cycle, along with a 76-year oscillation in its volume. NASA’s
orbiting SoHo observatory during the 1990s revealed a rapid five-minute
cycle of helioseismographic activity—of sound waves resonating
through the body of the sun (for details, see "Solar
and Stellar Activity Cycles" by
Peter R. Wilson).
biological organisms both also depend on feedback to maintain homeostasis,
or internal stability. The sun uses feedback controls specifically
to maintain its internal temperature, which must remain within a limited
range to keep the sun viable. If it were to cool excessively, the sun would
implode under its own gravity. If it were to heat up excessively, it
would fly apart. The sun keeps blazing because its tendency to expand—an
effect of its heat—is countered precisely by its tendency to
effect of its gravity. The temperature range at which these two
countervailing forces remain balanced corresponds to the range that keeps nucleosynthesis
proceeding in the way required for the sun to continue doing what it does.
the foregoing parallels between stellar and biological life, at least one essential biological process has no obvious
counterpart in the lives of stars. That process is reproduction. The star
larvae hypothesis fills the gap by accounting for the stellar reproductive
is addressed, ostensibly, by the standard scientific model of the stellar "life
When stars die, they do so explosively, expelling their bodily
material into the space around them. The death leaves behind a dense core,
which persists as a brown dwarf, neutron star, or black hole, depending
on the size of the original star. The material that is ejected into space enriches
nearby particle clouds, from which new stars form. This recycling
of material from one generation of stars to the next resembles reproduction. But it resembles the fertilization of roots more than it does
the production of seeds. It is a reproductive pseudo-cycle.
The recycling of material from
old stars into new ones does not produce new unattached protons, which are the spores/seeds from which new stars develop.
larvae hypothesis proposes that stars reproduce in a way that
more nearly resembles biological reproduction, insofar as it comprises discernible stages, each transitioning into the next in a predictable developmental sequence. The hypothesis proposes that stars constitute only the adult phase of the organism's life cycle and that the cycle also includes a larval phase. As with some biological organisms, star larvae bear little resemblance to their adult form.
Once bacteria and viruses arrive on a suitable planet the
larval phase of the stellar life cycle—biology—unfolds.
The larvae exploit the planetary resources,
and their population over time differentiates to include a type that on Earth goes by the name Homo sapiens and that is equipped by its nature to initiate the next vital phase of the stellar life cycle. This
avant-garde type constructs from the material resources of the incubator planet
complex niches—cities. It evolves
symbiotically with its evolving technologies and becomes highly
domesticated—neotenous. Eventually, the larvae migrate to new ecological niches that they construct in the orbital space around the incubator planet. The move to orbital —weightless—niches triggers a mutation/metamorphosis in the larvae. They develop into the next stage of the stellar life cycle, what might be called the angelic stage.
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