Date: 5/22/02 9:13:50 AM Pacific Daylight Time
Kent,I ran across this today:
http://space.com/scienceastronomy/astronomy/brown_dwarfs_020522.html
Is this the beginning of disclosure? Seems as thought it fits the bill for Planet X. Whatcha think?
5/22/02 7:28:12 PM Pacific Daylight Time
Hi Kent,
I lurk frequently in alt.astronomy and pick up some
interesting things
that are published by JPL - NASA's Ron Baalke, and the one posted in this
morning's lot was the one I've pasted below. The direction of the brown
dwarf being in Orion is where there are too many pointers for the return
of Nibiru appearing from the Orion direction for it to be a coincidence
surely. The first paragraph's "Is it a young planet, or a wandering old
brown dwarf in the line of sight?" is surprisingly speculative, especially
the 'line of sight' meaning that it is possibly anywhere between the stars
it seems to be near and Earth, and may be the same 'wanderer' that lensed
the background stars it was passing in front of last June, and said to have
puzzled the observers then, but I haven't yet read of any followup to that
news since it was published. I can't for the life of me imagine that the
news of such significance as a pass over of a brown dwarf will be shouted
from the rooftops, and all the shit that's going down around the world to
distract us by invoking national security bullshit and military control
does not seem to be a coincidence. What's below is certainly tantalising.
Sydney NSW Australia
----------------------------------------------------------------------------
Subject: Astronomers Ponder The Nature Of An Ultracool
Object In Orion
Date: 22 May 2002 16:52:08 GMT
From: baalke@zagami.jpl.nasa.gov (Ron Baalke)
Organization: Jet Propulsion Lab
Newsgroups: alt.sci.planetary, alt.astronomy
Institute for Astronomy
University of Hawaii
Honolulu, Hawaii
Contacts:
Dr. Eduardo Martin, 808-956-8637, ege@ifa.hawaii.edu
Mrs. Karen Rehbock, 808-956-6829, rehbock@ifa.hawaii.edu
For Immediate Release: May 20, 2002
ASTRONOMERS PONDER THE NATURE OF AN ULTRACOOL OBJECT IN ORION
A new substellar object, named SOri70, has been discovered near the
young star Sigma Orionis. Is it a young planet, or a wandering old
brown dwarf in the line of sight? This is a question to be discussed
by the astronomers attending the International Astronomical Union
Symposium on Brown Dwarfs that opens today on the Big Island of Hawaii.
Deep sky images and follow-up spectroscopy obtained by an international
team of astronomers revealed this extremely cool and dim object close
to the multiple stellar system Sigma Orionis. The astronomers made the
observations with large telescopes in Hawaii and the Canary Islands.
Since the acute visual observations of Sir William Herschel in the
eighteenth century, astronomers have noted a clustering of stars in a
region of the sky of about the size of the full moon surrounding the
hot star Sigma Orionis. Many X-ray emitting low-mass stars in this
cluster were found by Scott Wolk and Fred Walter of SUNY at Stony
Brook. Several brown dwarfs in this region were revealed by some of
the members of the team that today reports on the discovery of the
coolest and faintest object ever seen around Sigma Orionis.
The story of how SOri70 was found includes two of the world's most
powerful telescopes separated by more than 8,000 miles and about 4
years of international collaborative effort. It is an example of the
complicated work that is needed to hunt for the elusive brown dwarfs
and extrasolar planets.
In December 1998, team members Victor Bejar and Eduardo Martin
pointed one of the world's largest optical telescopes, the 10-meter
Keck I on Mauna Kea (Hawaii), at several fields around Sigma Orionis
and obtained CCD images of unprecedented sensitivity for this region
of the sky. They found several extremely faint red objects, but they
did not have enough information to determine their basic properties.
They had to wait patiently for a chance to obtain additional data.
It came when they used an infrared camera at the William Herschel
Telescope in La Palma (Canary Islands) in November 2000.
One of the objects turned out to have blue infrared colors despite
being very red at optical wavelengths, a unique signature of the
coolest known dwarfs. The unusual colors of these dwarfs are
explained by the presence of methane in their atmospheres, which
is a gas that can be present only at temperatures lower than about
1,200 degrees Kelvin (about 900 degrees Celsius or 1650 degrees
Fahrenheit). An object of this temperature must have a mass smaller
than a star.
The intriguing object was observed once more with the Keck I
telescope in December 2001 by team member Maria Rosa Zapatero Osorio
of the Laboratory for Fundamental Astrophysics in Madrid, Spain.
These observations confirmed spectroscopically the presence of
methane in the object, which unambiguously classifies it as a brown
dwarf or planet. If the object is located at the same distance as
the Sigma Orionis system (1,150 light-years from Earth), it should
have an age between 1 and 8 million years and a mass close to that
of Jupiter, the largest planet in the Solar System.
However, the distance to the object is not known yet; it will take
the sharp imaging capabilities of the Hubble Space Telescope to
determine it. There is about a 20% probability that SOri70 is a
wandering old brown dwarf that happens to be in the direction of
the Sigma Orionis, but is actually closer to Earth.
If the new ultracool dwarf is related to the Sigma Orionis system, it
would be the lowest mass extrasolar object imaged to date. Because it
would be located more than 180,000 astronomical units from Sigma
Orionis (more than 36,000 times the Jupiter-Sun distance), it would
challenge our ideas about the formation of extrasolar giant planets.
Four members of the science team are attending the International
Astronomical Union Symposium on Brown Dwarfs on the Big Island of
Hawaii during this week, namely, Dr. David Barrado y Navascues
(Laboratory for Fundamental Astrophysics in Madrid, Spain), Mr. Jose
Antonio Caballero (Instituto de Astrofisica de Canarias), Prof.
Eduardo Martin (University of Hawaii Institute for Astronomy) and Dr.
Maria Rosa Zapatero Osorio (Laboratory for Fundamental Astrophysics
in Madrid, Spain). Other team members include Dr. Victor Bejar
(Instituto de Astrofisica de Canarias), Dr. Joachim Eisloeffel
(Thueringer Landessternwarte Tautenburg, Germany), Dr. Reinhold
Mundt (Max Plank Institut fur Astronomie, Heidelberg, Germany), and
Dr. Rafael Rebolo (Instituto de Astrofisica de Canarias).
Members of the press and news media are invited to attend all
sessions of the Symposium at no cost. They are asked to check in at
the Conference Registration Desk at the Outrigger Waikoloa Beach
Hotel in order to obtain Symposium materials and other information
of interest.
More information about the Brown Dwarfs Symposium is available at
http://anansi.ifa.hawaii.edu/iau211/
The Institute for Astronomy at the University of Hawaii conducts
research into galaxies, cosmology, stars, planets, and the Sun. Its
faculty and staff are also involved in astronomy education, deep
space missions, and in the development and management of the
observatories on Haleakala and Mauna Kea. Refer to
http://www.ifa.hawaii.edu for more information.
Images:
An image of the Sigma Orionis region. The multiple star Sigma Orionis,
which is visible with the naked eye, is at the center. A box indicates
the position of the planet candidate, which is only 8.7 arcminutes
from the star. The image was taken from the Digital Sky Survey and
has a size of 23 x 22 square arcminutes. The inset shows the infrared
image obtained at the William Herschel Telescope by Dr. Victor Bejar
and Prof. Eduardo Martin.
* High-resolution color for offset press (tif file; 6,897K)
http://www.ifa.hawaii.edu/info/press-releases/brwnDwarf_300cmyk.tif
* High-resolution grayscle for offset press (tif file; 1,727K)
http://www.ifa.hawaii.edu/info/press-releases/brwnDwarf_300gray.tif
* Small jpeg for Web (23K)
http://www.ifa.hawaii.edu/info/press-releases/brwnDwarf_250web.jpg
* Large jpeg for Web (58K)
http://www.ifa.hawaii.edu/info/press-releases/brwnDwarf_480web.jpg
 |
Hmmmm, conference: NEW LIGHT ON THE DARKEST DWARFS Planet X maybe? 2 3 4 5 6 There are few big boards in Moscow with this image on it. The title is "New planet is approaching" Mark Hazelwood Agarthian Star Consciousness |
MORE NEWS! - Nibiru
Billboard 
EGADS! CROP CIRCLE!
PIONEER PROBE FROM THE NEW ILLUSTRATED SCIENCE AND INVENTION ENCYCLOPEDIA
MEMOS FROM
THE COMMANDER: The Hopi, and many ancient
cultures world wide, believe that when this 'event' occurs, all things made
by man return to the original state they came from. Anything not made of
stone or wood are gone in this belief system. Many Hopi keep housing made
only of earth and wood. They live in bi-levels and mobile homes but keep
a place to live in where its forbidden to even use nails. These cultures
also believe they can 'leave' during this event. As far as what is possible
and what is not, all bets are off when a brown dwarf star swings past your
planet, coming and going.
EDITOR: If some of the speculation above is true, sometimes I wonder if the Elites plan an evacuation? I don't think they'll make it in a bucket o' bolts. Maybe there's another way--a portal?
Far to the stars I journeyed until space and time became as naught. Then having drunk deep of the cup of wisdom, I looked into the hearts of men and there found I greater mysteries and was glad. For only in the Search for Truth could my Soul be stilled and the flame within be quenched. THOTH
