Life could possibly evolve on a neutron star itself
as “hyper-dense microscopic organisms controlled by nuclear forces with a
metabolism faster than ordinary chemical-based life,” suggests Lord Martin
Rees, Britain’s acclaimed Astronomer Royal and Cambridge University physicist. “Even if simple life is common, it is a separate question
whether it’s likely to evolve into anything we might recognize as intelligent
or complex – and where this might happen.”
Rees adds. But he warns: “If there’s advanced life
elsewhere we must not be too anthropomorphic about it. It may be something that
we would not recognize.”
Not so oddly, radio astronomer Frank Drake (of
Drake’s Equation fame) has suggested that intelligent life could inhabit
neutron stars, which inspired science-fiction author Robert Forward’s classic,
Dragon’s Egg, that developed Drake’s theory that such creatures would be
microscopic. It’s a story of sacrifice and triumph, human scientists establish
a relationship with intelligent lifeforms–the cheela–living on Dragon’s Egg, a
neutron star where one Earth hour is equivalent to hundreds of their years. The
cheela culturally evolve from savagery to the discovery of science, and for a
brief time, humans are their diligent teachers.
In 1991, radio signals from the pulsar PSR B1257+12
in the constellation Virgo led Penn State professor of Astronomy and
Astrophysics Alexander Wolszczan to the discovery of the first planets ever
known outside our solar system.
Wolszczan used the worlds largest radio telescope in
Arecibo, Puerto Rico, to time the radio signals coming from a distant tiny
neutron star in the constellation Virgo, 7,000 trillion miles from Earth. These
measurements helped him to determine that two of the planets are similar in
mass to Earth and the other is about the mass of the Moon.
In 2011, a former white dwarf star was discovered transformed into a
planet made of diamonds while circling a rapidly spinning pulsar. This dazzling
discovery was made using the 64 metre Parkes radio telescope in Australia where
irregularities in the signal from the pulsar alerted astronomers that something
was orbiting it. After follow up observations were made with the Lovell radio
telescope in the UK and one of the Keck telescopes in Hawaii, the international
team realised that there is something very unusual about this mysterious
object.
Until Wolszczan’s discovery, the only known planets were
in our solar system. The planets Wolszczan found probably don’t support life
because the tiny pulsar they orbit bombards them with deadly radiation.
The neutron star Wolszcan discovered is the remnant of a
supernova explosion–with a mass larger than the Sun’s compressed within a
radius of 10 kilometers with density 100 trillion times higher than an ordinary
solid.
The radiation neutron stars emit is exponentially
brighter than a terrestrial laser and its magnetic fields are millions times
more intense than what can be created in Earth-based labs along with gravity a
1000 billion times stronger than on Earth.
Wolszczan’s neutron star
radiates little light, but it emits penetrating x -rays and ejects winds at
nearly the speed of light.
Astronomers are baffled at how this planetary system got
there. But current thinking is that the earlier star had its own system of
planets before its supernova phase. The three remaining planets existed on the
outer orbits, possibly with life forms that would have been snuffed out by the
vaporizing blast of the supernova.
All three pulsar planets are shown in the image below;
the farthest two from the pulsar (closest in this view) are about the size of
Earth. Radiation from charged pulsar particles would probably rain down on the
planets, causing their night skies to light up with auroras similar to our
Northern Lights. One such aurora is illustrated on the planet at the bottom of
the picture.
Since this landmark discovery, more than 160 extrasolar
planets have been observed around stars that are burning nuclear fuel. The
planets spotted by Wolszczan might be part of a second generation of planets,
the first having been destroyed when their star blew up. The Spitzer Space
Telescope’s discovery of a dusty disk around a pulsar might represent the
beginnings of a similarly “reborn” planetary system.
A team led by Roberto Mignani from INAF Milan (Italy) and
from the University of Zielona Gora (Poland), used ESO’s Very Large Telescope
(VLT) at the Paranal Observatory in Chile to observe the neutron star RX
J1856.5-3754, about 400 light-years from Earth shown at top of the page.
Despite being amongst the closest neutron stars, its
extreme dimness meant the astronomers could only observe the star with visible
light using the FORS2 instrument on the VLT, at the limits of current telescope
technology.
Via DailyGalaxy
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