Natural Science Forum / Biology / Paleontology / March 2005

-------- Original Message --------
Subject:     Popcorn Supernovas-> mutagenic radiation in Australopithecus'
time ( pictures in the link)
Date:     Thu, 17 Mar 2005 06:39:41 -0800
From:     Roger Bagula <rlbagulatftn@yahoo.com>
To:     Quad- A <Quad-A@yahoogroups.com>, caveman <cavemen@yahoogroups.com>

Popcorn Supernovas    
   
   

A NASA mission launched in Mid-January 2003 is studying the remains of
some uncomfortably close supernova explosions.

by Dr Tony Phillips

Australopithecus squinted at the blue African sky. He had never seen a
star in broad daylight before, but he could see one today. White.
Piercing. Not as bright as the Sun, yet much more than a full moon. Was
it dangerous? He stared for a long time, puzzled, but nothing happened,
and after a while he strode across the savanna unconcerned.

Millions of years later, we know better.

"That star was a supernova, one of many that exploded in our part of the
galaxy during the past 10 million years," says astronomer Mark Hurwitz
of the University of California-Berkeley.

Supernovas near Earth are rare today, but during the Pliocene era of
Australopithecus supernovas happened more often. Their source was an
interstellar cloud called "Sco-Cen" that was slowly gliding by the solar
system. Within it, dense knots coalesced to form short-lived massive
stars, which exploded like popcorn.

Researchers estimate (with considerable uncertainty) that a supernova
less than 25 light years away would extinguish much of the life on
Earth. The blast needn't incinerate our planet. All it would take is
enough cosmic rays to damage the ozone layer and let through lethal
doses of ultraviolet (UV) radiation. Our ancestors survived the Pliocene
blasts only because the supernovas weren't quite so close.

We know because we can still see the cloud today. It's 450 light years
from Earth and receding in the direction of the constellations Scorpius
and Centaurus (hence the cloud's name, "Sco-Cen"). Astronomer Jesús
Maíz-Apellániz of Johns Hopkins University have backtracked Sco-Cen's
motion and measured its closest approach: 130 light years away about 5
million years ago.

Sco-Cen was still nearby only two million years ago when many plankton,
mollusks, and other UV-sensitive marine creatures on Earth mysteriously
died. Paleontologists mark it as the transition between the Pliocene and
Pleistocene epochs. Around the same time, according to German scientists
who have examined deep-sea sediments from the Pliocene era, Earth was
peppered with Fe60, an isotope produced by supernova explosions.

Coincidence?

No one knows. It's a puzzle researchers are still piecing together.

Reconstructing the history of near-Earth supernovas is difficult because
old supernovas are elusive. Their glowing shells fade to invisibility in
not much more than a million years. Neutron stars, the collapsed cores
of supernova progenitors, last longer, but they are flung across the
galaxy by asymmetries in the explosion. Unusual isotopes of iron, like
the ones that coincide with the marine extinction, are difficult to find
buried under millions of years of sediments.

There is, however, one obvious relic: "All those explosions blew an
enormous bubble in the interstellar medium," says Hurwitz, "and we're
inside it."

Astronomers call it "the Local Bubble." It's peanut-shaped, about 300
light years long, and filled with almost nothing. Gas inside the bubble
is very thin (0.001 atoms per cubic centimeter) and very hot (a million
degrees) - that's 1000 times less dense and 100 to 100,000 times hotter
than ordinary interstellar material.

The Local Bubble was discovered gradually in the 1970's and 1980's.
Optical and radio astronomers looked carefully for interstellar gas in
our part of the galaxy, but couldn't find much in Earth's neighborhood.
Furthermore, there seemed to be a pileup of gas - like the shell of a
bubble - about 150 light years away. Meanwhile, x-ray astronomers were
getting their first look at the sky using orbiting satellites, which
revealed a million-degree x-ray glow coming from all directions. "We
eventually realized that the solar system was inside a hot, vacuous
bubble," says Hurwitz.

In response, NASA launched a satellite in January 2003 - the Cosmic Hot
Interstellar Plasma Spectrometer, or "CHIPS" - to study the Local
Bubble. "There's a great deal we don't know about it," says Hurwitz, who
is the mission's chief scientist. How old is the bubble? What is its
internal geography? How fast is it cooling? Data from CHIPS is helping
to answer these questions.

The CHIPS Logo

CHIPS orbits Earth and peers into the bubble using an ultraviolet (UV)
telescope. "The gas in the bubble is very bright at extreme UV
wavelengths around 170 Å," explains Hurwitz. Other satellites have
examined such UV light from the bubble, but CHIPS is better. It has a
spectrometer on board with 100 channels ranging from 90 Å to 260 Å. "The
spectrometer is the key," he says.

Like sediments in the Pacific Ocean, gas in the Local Bubble contains
supernova-produced iron. "Iron atoms in the bubble have lost many of
their electrons - knocked loose by collisions within the hot gas."
CHIPS's spectrometer is able to detect spectral lines from iron atoms
missing 8, 9, 10 and 11 electrons, respectively. By comparing the
intensity of those four spectra lines, researchers can map the
temperature and density of gas in the bubble.

"If we find a hot spot," says Hurwitz, "that might be the location of
the most recent supernova." The spectra also tells researchers how fast
the gas is cooling and thus how old different parts of the bubble might
be. A fast-cooling knot of gas which is still hot must be pretty young,
for example.

Exploring the internal geography of the bubble is important because what
lies inside could affect our planet's future.

During the past few million years, wispy filaments of interstellar gas
have drifted into the Local Bubble. Our solar system is immersed in one
of those filaments - the "local fluff," a relatively cool (7000 K) cloud
containing 0.1 atoms per cubic centimeter. By galactic standards, the
local fluff is not very substantial. It has little effect on Earth
because the solar wind and the Sun's magnetic field are able to hold the
wispy cloud at bay.

more

An artist's concept of the local fluff
There are, however, denser clouds out there. The Sco-Cen complex, for
instance, is sending a stream of interstellar "cloudlets" in our
direction. "Some of those cloudlets might be hundreds of times denser
than the local fluff," says Priscilla Frisch, an astrophysicist at the
University of Chicago who studies the local interstellar medium. "If we
ran into one, it would compress the Sun's magnetic field and allow more
cosmic rays to penetrate the inner solar system, with unknown effects on
climate and life."

CHIPS is able to locate dense interstellar clouds by the shadows they
cast. Cool clouds are partially opaque to the bubble's UV glow, so they
appear as darker areas in CHIPS maps. Hurwitz notes that the mission's
first sky maps are rather coarse, with a resolution of 5o x 25o. (The
bowl of the Big Dipper, for comparison, is about 10 degrees wide.) Only
the largest clouds would appear in those. Later, if the mission is
extended beyond its first year, CHIPS will have time to produce sharper
maps with 5o x 6o resolution.

Frisch has noted that Homo Sapiens arose only after the local
interstellar medium was cleared out. Fewer clouds to run into would
promote a stabler climate for our planet, she argues. So perhaps what
Australopithecus saw was a good omen, after all....

CHIPS is helping us to find out.

http://www.firstscience.com/site/articles/supernovas.asp