Showing posts with label NRO. Show all posts
Showing posts with label NRO. Show all posts

Wednesday, June 13, 2012

Low cost development and applications of the new NRO donated telescopes, Page 3.

Copyright 2012 Robert Clark

Credit: NASA/JPL-Caltech/UCLA. This is a mosaic of the images covering the entire sky as observed by the Wide-field Infrared Survey Explorer (WISE), part of its All-Sky Data Release.  

 The WISE mission has released all the images taken during the duration of the mission:

NASA Releases New WISE Mission Catalog of Entire Infrared Sky.
03.14.12

"Today, WISE delivers the fruit of 14 years of effort to the astronomical community," said Edward Wright, WISE principal investigator at UCLA, who first began working on the mission with other team members in 1998.
WISE launched Dec. 14, 2009, and mapped the entire sky in 2010 with vastly better sensitivity than its predecessors. It collected more than 2.7 million images taken at four infrared wavelengths of light, capturing everything from nearby asteroids to distant galaxies. Since then, the team has been processing more than 15 trillion bytes of returned data. A preliminary release of WISE data, covering the first half of the sky surveyed, was made last April.
The WISE catalog of the entire sky meets the mission's fundamental objective. The individual WISE exposures have been combined into an atlas of more than 18,000 images covering the sky and a catalog listing the infrared properties of more than 560 million individual objects found in the images. Most of the objects are stars and galaxies, with roughly equal numbers of each. Many of them have never been seen before.
http://www.nasa.gov/mission_pages/WISE/news/wise20120314.html

WISE Delivers Millions of Galaxies, Stars, Asteroids.
04.14.11
Astronomers across the globe can now sift through hundreds of millions of galaxies, stars and asteroids collected in the first bundle of data from NASA's Wide-field Infrared Survey Explorer (WISE) mission.
"Starting today thousands of new eyes will be looking at WISE data, and I expect many surprises," said Edward (Ned) Wright of UCLA, the mission's principal investigator. 

The Wide-field Infrared Survey Explorer
All-Sky Data Release
March 14, 2012

 The WISE mission has made many important discoveries: 

WISE Finds Few Brown Dwarfs Close to Home.
June 08, 2012
WISE was launched in 2009 and surveyed the entire sky in infrared light in 2010. One of the mission's main science goals was to survey the sky for the elusive brown dwarfs. These small bodies start their lives like stars, but lack the bulk required to burn nuclear fuel. With time, they cool and fade, making them difficult to find. 
Improvements in WISE's infrared vision over past missions have allowed it to pick up the faint glow of many of these hidden objects. In August 2011, the mission announced the discovery of the coolest brown dwarfs spotted yet, a new class of stars called Y dwarfs. One of the Y dwarfs is less than 80 degrees Fahrenheit (25 degrees Celsius), or about room temperature, making it the coldest star-like body known. Since then, the WISE science team has surveyed the entire landscape around our sun and discovered 200 brown dwarfs, including 13 Y dwarfs. 

NASA Survey Counts Potentially Hazardous Asteroids.
May 16, 2012
PASADENA, Calif. -- Observations from NASA's Wide-field Infrared Survey Explorer (WISE) have led to the best assessment yet of our solar system's population of potentially hazardous asteroids. The results reveal new information about their total numbers, origins and the possible dangers they may pose.
Potentially hazardous asteroids, or PHAs, are a subset of the larger group of near-Earth asteroids. The PHAs have the closest orbits to Earth's, coming within five million miles (about eight million kilometers), and they are big enough to survive passing through Earth's atmosphere and cause damage on a regional, or greater, scale.
The new results come from the asteroid-hunting portion of the WISE mission, called NEOWISE. The project sampled 107 PHAs to make predictions about the entire population as a whole. Findings indicate there are roughly 4,700 PHAs, plus or minus 1,500, with diameters larger than 330 feet (about 100 meters). So far, an estimated 20 to 30 percent of these objects have been found.
While previous estimates of PHAs predicted similar numbers, they were rough approximations. NEOWISE has generated a more credible estimate of the objects' total numbers and sizes.
"The NEOWISE analysis shows us we've made a good start at finding those objects that truly represent an impact hazard to Earth," said Lindley Johnson, program executive for the Near-Earth Object Observation Program at NASA Headquarters in Washington. "But we've many more to find, and it will take a concerted effort during the next couple of decades to find all of them that could do serious damage or be a mission destination in the future."

in addition to the searches for nomad planets and hypothesized planets at the edge of the Solar System: 

Can WISE Find the Hypothetical 'Tyche'?
February 18, 2011
Frequently Asked Questions
Q: When could data from WISE confirm or rule out the existence of the hypothesized planet Tyche?
A: It is too early to know whether WISE data confirms or rules out a large object in the Oort cloud. Analysis over the next couple of years will be needed to determine if WISE has actually detected such a world or not. The first 14 weeks of data, being released in April 2011, are unlikely to be sufficient. The full survey, scheduled for release in March 2012, should provide greater insight. Once the WISE data are fully processed, released and analyzed, the Tyche hypothesis that Matese and Whitmire propose will be tested.

  With the release of the image database, to help with the search for brown drawfs, potentially harmful asteroids, nomad planets, and extreme Solar System planets I recommend the use of distributed computing such as that used for the Seti@Home project to allow potentially millions of people to take part in the searches. With the great interest in the public in extraterrestrial life and possible Earth impacting asteroids, and with the possibility of discovering a new Solar System planet, there very likely would be a great deal of interest in such a project.

 And with asteroid mining ventures needing to find high value asteroids nearby, they could offer prizes, i.e., rewards, for those users who happened to find them.


  Bob Clark

Tuesday, June 12, 2012

Low cost development and applications of the new NRO donated telescopes, Page 2.

Copyright 2012 Robert Clark 
Credit: NASA simulated image of extreme Solar System bodies


Hubble-class scopes can be placed at GEO rather than a Lagrangian point.

The Planetary Resources, Inc. version of such an infrared scope would operate in low Earth orbit. Then it quite likely could be launched by a Falcon 9, at a ca. $50 million launch cost. However, the plans for the Wide Field Infrared Survey Telescope (WFIRST) that these NRO scopes could be used for would be to place it at a Sun-Earth Lagrangian point millions of miles away. But according to this article the large size of these new scopes would allow them to be placed much nearer, in geosynchronous orbit:

Ex-Spy Telescope May Get New Identity as a Space Investigator.
By DENNIS OVERBYE
Published: June 4, 2012

The telescope’s short length means its camera could have the wide field of view necessary to inspect large areas of the sky for supernovae.
Even bigger advantages come, astronomers say, from the fact that the telescope’s diameter, 94 inches, is twice as big as that contemplated for Wfirst, giving it four times the light-gathering power, from which a whole host of savings cascade.
Instead of requiring an expensive launch to a solar orbit, the telescope can operate in geosynchronous Earth orbit, complete its survey of the sky four times faster, and download data to the Earth faster.
Equipped with a coronagraph, which blocks light from the sun’s disk to look for exoplanets, another of Wfirst’s goals, the former spy telescope could see planets down to the size of Jupiter around other stars.
http://www.nytimes.com/2012/06/05/science/space/repurposed-telescope-may-explore-secrets-of-dark-energy.html

 Then they could be launched at least by a Falcon Heavy at a $100 million launch cost. The colder temperatures out at GEO compared to LEO would make the PRI asteroid search more sensitive also.


Cost advantage of a single large scope compared to multiple small scopes.

 In regards to PRI financing the development of such a scope, PRI has announced plans to make small telescopes of about 9" diameter to be sold for Earth imaging purposes and to combine hundreds to thousands of these for the asteroid search:

APRIL 26, 2012
Planetary Resources could take megapixel images of exoplanet and makes billions by 2020 before mining anything.
http://nextbigfuture.com/2012/04/planetary-resources-could-use-passively.html



However, linking up optical or infrared telescopes in orbit to form a single coherent image has not been done before and likely will add significantly to the price of the individual scopes. If it does work then the resolution will be as the widest distance between the scopes. However the light collecting area, which is what is needed for the sensitivity of an asteroid search, will only be as the sum of the areas of the scopes.
 The new NRO scopes have 11 times the diameter of the planned PRI telescopes. So it would take 121 of the PRI scopes to make up the sensitivity of a single one of the NRO scopes, assuming they are able to get a single coherent image from the combined scopes. 
 PRI has said they expect to cut the costs of their scopes by 1 to 2 orders of magnitude below that of, for example, a telescope as on the WISE mission. This would make them in the $3 to $30 million dollar range. With the complexity of the wide scale link up of the scopes at hundreds to thousands of kilometer distances,  it seems likely it would be closer to the higher range. Even if the Arkyds amount to $10 million each including launch costs, that would still be over a billion dollars to match the sensitivity of a single one of the NRO  scopes. In that case a single one of the NRO scopes at a few hundred million dollar cost would be advantageous.


The Hubble-class scopes properly instrumented can serve as upgrades both for the WISE and WFIRST scopes. 

 Interesting articles here about the WISE capability to detect large unknown planets at the very fringes of the Solar System:

Up telescope! Search begins for giant new planet.Tyche may be bigger than Jupiter and orbit at the outer edge of thesolar system. BY PAUL RODGERS SUNDAY 13 FEBRUARY 2011
http://www.independent.co.uk/news/science/up-telescope-search-begins-for-giant-new-planet-2213119.html

About that Giant Planet Possibly Hiding in the Outer Solar System...by NANCY ATKINSON on FEBRUARY 16, 2011
http://www.universetoday.com/83363/about-that-giant-planet-possibly-hiding-in-the-outer-solar-system/

 The 40 times greater collecting area means the Hubble-class scopes could perform a much more sensitive search than WISE for these extreme Solar System planets.
 Another possible use would be the search for nomad or rogue planets which are planets in the interstellar space between star systems:

Researchers say galaxy may swarm with 'nomad planets'. A good count, especially of the smaller objects, will have towait for the next generation of big survey telescopes, especially thespace-based Wide-Field Infrared Survey Telescope and the ground-based Large Synoptic Survey Telescope, both set to begin operation in theearly 2020s. A confirmation of the estimate could lend credence to another possibility mentioned in the paper - that as nomad planets roam theirstarry pastures, collisions could scatter their microbial flocks to seed life elsewhere. February 23, 2012 BY ANDY FREEBERG
http://phys.org/news/2012-02-galaxy-swarm-nomad-planets.html

 Again the Hubble-class scopes would have much better sensitivity to detect them than the Wide-Field Infrared Survey Telescope(WFIRST) scope mentioned.
 It has been speculated such nomad planets could have life in subsurface water. Since some of these nomads are believed to be ejected from other star systems, nomads near to us or captured by our Solar System would provide a more near term route to search for life in other star systems.
 Because of the interest in the search for extraterrestrial life, you could have another source for private funding for such scopes. One could have for example the scope named after a foundation or individual who provided a large portion of the funding, like the Keck telescope.



   Bob Clark


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