Untitled Essay Research Paper BETA PICTORIS PLANETS

Untitled Essay, Research Paper BETA PICTORIS: PLANETS? LIFE? OR WHAT?JARAASTRONOMY The ultimate question is; Is there a possibility that life might exist on a planet in the

Untitled Essay, Research Paper


The ultimate question is; Is there a possibility that life might exist on a planet in the

Beta Pictoris system? First, one must ask, Are there planets in the Beta Pictoris system?.

However, that question would be impossible to answer if one did not answer the most basic

questions first; Where do planets come from? and do the key elements and situations,

needed to form planets, exist in the Beta Pictoris system?.

To understand where planets come from, one has to first look at where the planets in our

solar system came from. Does or did our star, the sun, have a circumstellar disk around

it? the answer is believed to be yes.

Scientists believe that a newly formed star is immediately surrounded by a relatively

dense cloud of gas and dust. In 1965, A. Poveda stated, “That new stars are likely to

be obscured by this envelope of gas and dust (1).” In 1967, Davidson and Harwit

agreed with Poveda and then termed this occurrence, the “cocoon nebula” (1).

Other authors have referred to this occurrence as, a “placental nebula” (1),

noting that it sustains the growth of planetary bodies.

For a long time, even before there was the term cocoon nebula, planetary scientists knew

that a cocoon nebula had surrounded the sun, long ago, in order for our solar system to

form and take on their currents motions (1).

In 1755, a German, named Immanuel Kant, reasoned that “gravity would make circumsolar

cloud contract and that rotation would flatten it (1)." Thus, the cloud would assume

the general shape of a rotating disk, explaining the fact that the planets, in our solar

system, revolve in a disk-shaped distribution.

This idea, about the disk-shaped nebula that was formed around the early sun, came to be

known as the nebula hypothesis (1). Then, in 1796, a French mathematician named Laplace,

proposed that the rotating disk continued to cool and contract, forming planetary bodies

(1). Also, when investigating the evolution of stars, it was proposed “that a star

forms as a central condensation in an extended nebula… The outer part remains behind as

the cocoon nebula (1)”. During the same study it was also indicated that under

various conditions such as: rotation, turbulence, etc. the nucleus of the forming star may

divide into two or more bodies orbiting each other (1). This may be the explanation as to

why more than half of all star systems are binary or multiple, rather than singles stars,

like ours, the sun.

This same fragmentation may also form bodies too small to become stars. However, they

could form into large planets, about the same size as Jupiter (1).

In 1966, Low and Smith calculated that the dust must be orbiting the star at a distance of

many tens of astronomical units, in order for planets to from (1). Others have reasoned

that the cocoon nebula must contain silicate and/or ice particles (planet-forming

materials), in order for the presence of planetary bodies (1). Still others have concluded

that planets form during the early life of a star (1).

After determining that planets are formed in a circumstellar disk surrounding a star, we

must ask ourselves, Does Beta Pictoris have a cirumstellar disk around it?

Beta Pictoris was found to have a circumstellar disk in 1983. It was first detected by the

Infrared Astronomy Satellite. The disk is seen to extend to more than 400 astronomical

units from the star (2). The orbits of most of the particles are inclined 5 degrees or

less to the plane of the system (2). These minimal orbital inclinations are typical of the

major planets in our own solar system. There is evidence that the circumstellar material

around Beta Pictoris takes the form of a highly flattened disk, rather than a spherical

shell implies an almost certain association with planet formation (2). The disk material

itself is believed to be a potential source for planet accretion (2). This retention of

nearly coplanar orbits in the Beta Pictoris disk is a qualitative argument in support of

its being a relatively young system (2). Some astronomers believe that we are witnessing

planet formation in the process.

Lagage and Pantin found that the inner region of the disk surrounding Beta Pictoris is

clear of dust, a prime indicator that there is evidence of one or more planetary bodies


The depletion zone extends to about 15 AU from the star, about the same size as our solar

system; and has an average particle density only one tenth of the area just outside this

zone (3).

Lagage and Pantin believe that the inner zone may have been swept clean by the

gravitational pull of a planet orbiting around Beta Pictoris (3). A planet would

gravitationally deflect the particles out of the inner zone. This planet, which is only

believed to exist, may also be deflecting comets into the star, as indicated by the

presence of highly variable absorption lines in the spectrum of Beta Pictoris (3).

The infrared image by Lagage and Pantin also provide information that the edge-on disk is

not symmetrical around the star (3). This suggests a more intimate relationship between

the asymmetry and the properties of the inner disk. As the orbital timescale for particles

is relatively short (less than 100 years), one would expect that the irregularities in the

disk would have been smoothed out by now (3). Unless, there was something stirring it up,

such as a planet (3).

If there is a planet orbiting Beta Pictoris, its orbit is probably eccentric, as are most

of the planetary orbits in our solar system (4). A planet with even a moderately eccentric

orbit would generate the asymmetry that is been noted in the dust disk surrounding Beat

Pictoris (4).

The Hubble Space Telescope, using the high-resolution spectrograph, found that the disk

surrounding beta Pictoris consists of two parts: an outer ring of small, solid particles,

and an inner ring of diffuse gas within a few hundred miles of the star (5).

Albert Boggess, an astronomer at NASA’s Goddard Space Flight Center, suspects that

the gas comes from the ring of solid particles (5). If he is correct, then the gas may be

a sign that planets are being born there. The gas could be a result from the collision of

solid particles in the outer ring accreting into planets that are still too small to see

because of the brightness of the star itself (5). During the collisions some of the

particles would be vaporized and drawn toward the star. The planets in our own solar

system are believed to have formed through countless numbers of such collisions (5).

Boggess also believes that Beta Pictoris is very similar to a very early phase of our own

solar system (5).

Additional evidence, from the Hubble, also suggests that Beta Pictoris might be following

in our footsteps. The gaseous inner ring appears to contain clumps of material spiraling

toward the star (5). These clumps may be comets, diverted from the normal paths by close

calls with protoplanets (5). This also fits with current ideas about the evolution of our

own solar system. Gases from comet impacts may have been the creating factor of the

Earth’s atmosphere and oceans (5).

Wetherill argues that life on Earth is reliant upon the existence of Jupiter and Saturn,

because they cleansed our Solar System of most of its planetesimals (comets) that,

otherwise, would be striking the Earth (6). In order for a planet to survive long enough

for life to begin, it is necessary for the existence of gas giants (Jupiter and Saturn) to

get rid of the hazardous comets.

No one person can say for sure whether there are planets in the Beta Pictoris System, or

not. However, it is definitely a possibility. There is a circumstellar disk surrounding

Beta Pictoris. It is a highly flattened disk, as was the disk that once surrounded the

Sun. The disk contains the necessary elements for planet formation. The star is a young

one. The inner zone of the disk is clear. All of these things point to the almost probable

formation of planets. Richard Terrile, from the Jet Propulsion Laboratory, says,

“It’s hard not to form planets from material like this (7).”

To answer whether or not there could be life on one of these planets, is not easy to say.

No one can really even speculate. I, believe that it is possible, if all the variables

come together in just the right way. I am not ‘earthnocentric’ to assume that

the earth is the only planet in the Universe that can sustain life. Whether or not a

planet in the Beta Pictoris system has what it takes, who knows, we can only wait and


BIBLIOGRAPHY(1) Moons And Planets, third edition; William K.

Hartman; Wadsworth Publishing company;

California; 1993.(2) A Circumstellar Disk Around Beta Pictoris; Science;

volume 226; pages 1421-1424.(3) Footprints in The Dust; Charles M. Telesco;

Nature; volume 369; pages 610-611.(4) Dust Depletion In The Inner Disk Of Beta Pictoris

As A Possible Indicator Of Planets; P. O. Lagage

and E. Pantin; Nature; volume 369; pages 628-

630.(5) Birth Of A Solar System?; Tim Folger; Discover;

volume 13; page 27.(6) Inhibition Of Giant-planet formation By Rapid Gas

Depletion Around Young Stars; B. Zucherman,

T. Forveille, and J. H. Kastner; Nature; volume

373; pages 494-496.(7) A Planet Around Beta Pictoris?; Sky and Telescope;

Volume 88; page 10.

ADDITIONAL BIBLIOGRAPHYA Closer Look At Beta Pictoris; Astronomy;

volume 21; Page 18.Birth Announcements; Scientific American;

volume 256; pages 60+.Faraway Planets; Science Digest; volume 94;

page 47.Protoplanetary nebula around Beta Pictoris;

Astronomy; volume 13; page 60.