Saturday, 17 January 2015

Ascension Earth 2012 -- January 17, 2015

Ascension Earth 2012


  • Pair of Dwarf Planets May Lurk Beyond Pluto in Our Solar System
  • Amazing time-lapse video of Earth shot from space
  • Move Over Hubble, Meet the New High Powered Star Searcher
  • The Best Bet for Alien Life May Be in Planetary Systems Very Different From Ours
  • How Well Do You Really Know Yourself?
  • One Step Beyond ~ Life After Death
  • The Drug War on Coast To Coast Radio with George Noory
  • The 5 Most Mysterious Objects in our Solar System
  • Largest star ever discovered, compared to our Sun
  • Babylonian Creation Myths ~ Studies in Comparitive Mythology ~ Manly P Hall
Posted: 16 Jan 2015 08:30 PM PST

planets

At least two unknown dwarf planets may be lurking beyond Pluto, orbiting around the Sun in our own solar system just waiting to be discovered, according to a new study. (Photo : NASA/JPL-Caltech)


Excerpt from natureworldnews.com

At least two unknown dwarf planets may be lurking beyond Pluto, orbiting around the Sun in our own solar system just waiting to be discovered, according to a new study.

This comes from an analysis of objects observed beyond Neptune, called extreme trans-Neptunian objects (ETNO), which normally should be flying around randomly in space, but in this case show some unusual symmetry.

"This excess of objects with unexpected orbital parameters makes us believe that some invisible forces are altering the distribution of the orbital elements of the ETNO," Carlos de la Fuente Marcos, with the Complutense University of Madrid, said in a press release.
"We consider that the most probable explanation is that other unknown planets exist beyond Neptune and Pluto," he added.

According to conventional theory, there is a certain set of characteristics that ETNO orbits must fulfill. For example, they should have a semi-major axis, or average distance from the Sun, of about 150 astronomical units (AU). (1 AU is the distance from Earth to the Sun - roughly 93 million miles, or 150 million kilometers.) These orbits should also have an inclination, relative to the plane of the solar system, of almost 0 degrees.

However, the actual orbits of the 13 ETNOs studied are quite different, with semi-major axes ranging from 150 to 525 AU and average inclinations of about 20 degrees.

"The exact number is uncertain, given that the data that we have is limited, but our calculations suggest that there are at least two planets, and probably more, within the confines of our solar system," Marcos said.

The new results are detailed in two papers in the journal Monthly Notices of the Royal Astronomical Society. 
Posted: 16 Jan 2015 08:21 PM PST





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Posted: 16 Jan 2015 08:16 PM PST

NASA'S James Webb Space Telescope


Excerpt from space.com

 
NASA's James Webb Space Telescope, scheduled for launch in 2018, will probe the cosmos to uncover the history of the universe from the Big Bang to alien planet formation and beyond.
Scientists are planning to use the infrared telescope to search for the first galaxies that formed at the beginning of the universe. The James Webb Space Telescope (JWST) will also have the ability to look through cosmic dust clouds to find newly forming planetary systems and seek out the chemical origins of life in the solar system.

The powerful $8.8 billion spacecraft is also expected to take amazing photos of celestial objects like its predecessor, the Hubble Space Telescope.

Instruments on board

The JWST will come equipped with four science instruments.
  • Near-Infrared Camera (NIRCam) — Provided by the University of Arizona, this infrared camera will detect light from stars in nearby galaxies and stars within the Milky Way. It will also search for light from stars and galaxies that formed early in the universe's life. NIRCam will be outfitted with coronagraphs that can block a bright object's light, making dimmer objects near those stars (like planets) visible.
  • Near-Infrared Spectrograph (NIRSpec) — NIRSpec will observe 100 objects simultaneously, searching for the first galaxies that formed after the Big Bang. NIRSpec was provided by the European Space Agency with help from NASA's Goddard Space Flight Center.
  • Mid-Infrared Instrument (MIRI) — MIRI will produce amazing space photos of distant celestial objects, following in Hubble's tradition of astrophotography. The spectrograph that is a part of the instrument will allow scientists to gather more physical details about distant objects in the universe. MIRI will detect distant galaxies, faint comets, forming stars and objects in the Kuiper Belt. MIRI was built by the European Consortium with the European Space Agency and NASA's Jet Propulsion Laboratory.
  • Fine Guidance Sensor/Near InfraRed Imager and Slitless Spectrograph (FGS/NIRISS) — This Canadian Space Agency-built instrument is more like two instruments in one. The FGS component is responsible for keeping the JWST pointed in exactly the right direction during its science investigations. NIRISS will scope out the cosmos to find signatures of the first light in the universe and seek out and characterize alien planets.
The telescope will also sport a tennis court-size sunshield and a 21.3 foot (6.5 meter) mirror — the largest mirror ever launched into space. Those components will not fit into the rocket launching the JWST, so both will unfurl once the telescope is in space.
Infrared: Inside the huge space observatory that operates from a point in space four times further away than the moon.
NASA's James Webb Space Telescope is an $8.8 billion space observatory built to observe the infrared universe like never before. See how NASA's James Webb Space Telescope works in this Space.com infographic
 
James Webb the man

The JWST is named for former NASA chief James Webb. Webb took charge of the space agency from 1961 to 1968, retiring just a few months before NASA put the first man on the moon.
Posted: 16 Jan 2015 08:08 PM PST



Excerpt from wired.com


In the hunt for extraterrestrial life, scientists started by searching for a world orbiting a star just like the sun. After all, the steady warmth of that glowing yellow ball in the sky makes life on Earth possible.

But as astronomers continue to discover thousands of planets, they’re realizing that if (or when) we find signs of extraterrestrial life, chances are good that those aliens will orbit a star quite different from the sun—one that’s redder, cooler, and at a fraction of the sun’s size and mass. So in the quest for otherworldly life, many astronomers have set their sights on these small stars, known as red dwarfs or M dwarfs.

At first, planet-hunting astronomers didn’t care so much about M dwarfs. After the first planet outside the solar system was discovered in 1995, scientists began hunting for a true Earth twin: a rocky planet like Earth with an orbit like ours around a sun-like star. Indeed, the search for that kind of system drove astronomers through most of the 2000s, says astronomer Phil Muirhead of Boston University.

But then astronomers realized that it might be technically easier to find planets around M dwarfs. Detecting another planet is really hard, and scientists rely on two main methods. In the first, they look for a drop in a star’s brightness when a planet passes in front of it. In the second, astronomers measure the slight wobble of a star, caused by the gentle gravitational tug of an orbiting planet. With both of these techniques, the signal is stronger and easier to detect for a planet orbiting an M dwarf. A planet around an M dwarf also orbits more frequently, increasing the chances that astronomers will spot it.

M dwarfs got a big boost from the Kepler space telescope, which launched in 2008. By staring at small patch of the sky, the telescope searches for suddenly dimming stars when a planet passes in front of them. In doing so, the spacecraft discovered a glut of planets—more than 1,000 at the latest count—it found a lot of planets around M dwarfs. “Kepler changed everything,” Muirhead said. Because M-dwarf systems are easier to find, the bounty of such planets is at least partly due to a selection effect. But, as Muirhead points out, Kepler is also designed to find Earth-sized planets around sun-like stars, and the numbers so far suggest that M-dwarfs may offer the best odds for finding life.

“By sheer luck you would be more likely to find a potentially habitable planet around an M dwarf than a star like the sun,” said astronomer Courtney Dressing of Harvard. She led an analysis to estimate how many Earth-sized planets—which she defined as those with radii ranging from one to one-and-a-half times Earth’s radius—orbit M dwarfs in the habitable zone, the region around the star where liquid water can exist on the planet’s surface. According to her latest calculations, one in four M dwarfs hosts such a planet.

That’s higher than the estimated number of Earth-sized planets around a sun-like star, she says. For example, an analysis by astronomer Erik Petigura of UC Berkeley suggests that fewer than 10 percent of sun-like stars have a planet with a radius between one and two times that of Earth’s.

This illustration shows Kepler-186f, the first rocky planet found in a star's habitable zone. Its star is an M dwarf.
This illustration shows Kepler-186f, the first rocky planet found in a star’s habitable zone. Its star is an M dwarf.  NASA Ames/SETI Institute/JPL-Caltech


M dwarfs have another thing going for them. They’re the most common star in the galaxy, comprising an estimated 75 percent of the Milky Way’s hundreds of billions of stars. If Dressing’s estimates are right, then our galaxy could be teeming with 100 billion Earth-sized planets in their stars’ habitable zones.

To be sure, these estimates have lots of limitations. They depend on what you mean by the habitable zone, which isn’t well defined. Generally, the habitable zone is where it’s not too hot or too cold for liquid water to exist. But there are countless considerations, such as how well a planet’s atmosphere can retain water. With a more generous definition that widens the habitable zone, Petigura’s numbers for Earth-sized planets around a sun-like star go up to 22 percent or more. Likewise, Dressing’s numbers could also go up.
Astronomers were initially skeptical of M-dwarf systems because they thought a planet couldn’t be habitable near this kind of star. For one, M dwarfs are more active, especially during within the first billion years of its life. They may bombard a planet with life-killing ultraviolet radiation. They can spew powerful stellar flares that would strip a planet of its atmosphere.

And because a planet will tend to orbit close to an M dwarf, the star’s gravity can alter the planet’s rotation around its axis. When such a planet is tidally locked, as such a scenario is called, part of the planet may see eternal daylight while another part sees eternal night. The bright side would be fried while the dark side would freeze—hardly a hospitable situation for life.

But none of these are settled issues, and some studies suggest they may not be as big of a problem as previously thought, says astronomer Aomawa Shields of UCLA. For example, habitability may depend on specific types and frequency of flares, which aren’t well understood yet. Computer models have also shown that an atmosphere can help distribute heat, preventing the dark side of a planet from freezing over.
Posted: 16 Jan 2015 07:55 PM PST


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To Gregg,

Resultado de imagem para thank you roses images

For all these years of Friendship,
Guidance and Enlightment.

Ascension Earth 2012

Farewell from Ascension Earth!

I would like to extend a heartfelt thank you to each and every one of you for visiting Ascension Earth over the past few years and making this site, what I consider, such a wonderful and very surprising success since my first post way back in January of 2011. I never dreamed this site would receive just shy of 10 million page views since then, and I want to thank you all again for stopping in from time to time for a visit. I hope you have found some of the content interesting as well as educational, and I want everyone to know that I only shared content I believed to be factual at the time of publication, though I may have reached differing understandingsconcerning some of the subject matter as time has past. All of the content that has been shared here at Ascension Earth was shared with the goal of provoking contemplation and conversation, leading to a raising of consciousness, an ascension of consciousness. That's what ascension is to me.

I have made a decision to move on from here, but I will always remember and always cherish the friendships I have made along this twisting journey since launching this site, what feels like a lifetime ago now. I wish all of you the greatest success in each and every endeavor you shall undertake, and I hope each of you are graced with peace, love & light every step of the way as you continue your never ending journey through this incredibly breathtaking and ever mysterious universe we share together.

Greg

Morgan Kochel says:

Conversation with
A Man Who Went to Mars
by Morgan Kochel

…And there you have it! This was the end of our discussion about the Mars mission, but I have remained in touch with Chad. At this point, I hope to be able to convince him to do a video or TV interview, but of course, there will be more than a few obstacles to overcome, the main one being that he may currently be in some danger if he goes public.

Furthermore, there is always the barrier of peoples' understandable skepticism.

As I said in the beginning, I cannot verify this story for anyone, nor is my intent to convince anyone of its veracity. My goal is only to help him get his story heard, because if this story IS true, the people of this planet are being lied to on a grand scale, and perhaps this will eventually help the UFO Disclosure Movement. It's time for the lies to be uncovered, and time for the truth -- whatever that may be -- to be known once and for all.

a man

esoteric



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