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

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

(3).

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

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