Tuesday, 24 May 2016
Saturday, 21 May 2016
NASA : Bigelow Expandable Activity Module
The Bigelow Expandable Activity Module (BEAM) is an expandable habitat technology demonstration for the International Space Station. Expandable habitats greatly decrease the amount of transport volume for future space missions. These “expandables” are lightweight and require minimal payload volume on a rocket, but expand after being deployed in space to potentially provide a comfortable area for astronauts to live and work. They also provide a varying degree of protection from solar and cosmic radiation, space debris, atomic oxygen, ultraviolet radiation and other elements of the space environment.
The journey to Mars is complex and filled with challenges that NASA and its partners are continuously working to solve. Before sending the first astronauts to the Red Planet, several rockets filled with cargo and supplies will be deployed to await the crews’ arrival. Expandable modules, which are lower-mass and lower-volume systems than metal habitats, can increase the efficiency of cargo shipments, possibly reducing the number of launches needed and overall mission costs.
Mission Highlights
- BEAM is scheduled to launch on the eighth SpaceX Commercial Resupply Service mission. After being attached to the Tranquility Node using the station’s robotic Canadarm2, it will be filled with air to expand it for a two-year test period in which astronauts aboard the space station will conduct a series of tests to validate overall performance and capability of expandable habitats.
- Crews will routinely enter to take measurements and monitor its performance to help inform designs for future habitat systems. Learning how an expandable habitat performs in the thermal environment of space and how it reacts to radiation, micrometeroids, and orbital debris will provide information to address key concerns about living in the harsh environment of space.
- Following the two-year test and validation period, BEAM will be robotically jettisoned from the space station, leaving orbit to burn during its descent through Earth’s atmosphere—much like many cargo spacecraft do.
- If BEAM performs favorably, it could lead to future development of expandable habitation structures for future crews traveling in deep space.
- The BEAM is an example of NASA’s increased commitment to partnering with industry to enable the growth of the commercial use of space. The BEAM project is co-sponsored by NASA's Advanced Exploration Systems (AES) Division and Bigelow Aerospace, which pioneers innovative approaches to rapidly and affordably develop prototype systems for future human exploration missions. The BEAM demonstration supports an AES objective to develop a deep space habitat for human missions beyond Earth orbit.
More about BEAM
01.16.13 - NASA Announces BEAM Plans
03.12.15 - BEAM Completes Major Milestones
08.27.15 - BEAM Facts, Figures and FAQs answered
Sunday, 15 May 2016
The WMAP
Wilkinson Microwave Anisotropy Probe :
From Wikipedia, the free encyclopedia
Artist's impression of WMAP
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Names | MAP Explorer 80 | ||||
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Mission type | CMBR Astronomy | ||||
Operator | NASA | ||||
COSPAR ID | 2001-027A | ||||
SATCAT № | 26859 | ||||
Website | map | ||||
Mission duration | 9 years, 1 month, 19 days | ||||
Spacecraft properties | |||||
Manufacturer | NASA / NRAO | ||||
Launch mass | 835 kg (1,841 lb)[1] | ||||
Dry mass | 763 kg (1,682 lb) | ||||
Dimensions | 3.6 m × 5.1 m (12 ft × 17 ft) | ||||
Power | 419 W | ||||
Start of mission | |||||
Launch date | 19:46:46, June 30, 2001[2] | ||||
Rocket | Delta II 7425-10 | ||||
Launch site | Cape Canaveral SLC-17 | ||||
End of mission | |||||
Disposal | passivated | ||||
Deactivated | October 28, 2010 | ||||
Orbital parameters | |||||
Reference system | L2 point | ||||
Regime | Lissajous | ||||
Main telescope | |||||
Type | Gregorian | ||||
Diameter | 1.4 m × 1.6 m (4.6 ft × 5.2 ft) | ||||
Wavelengths | 23 GHz to 94 GHz | ||||
Instruments | |||||
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Part of a series on |
Physical cosmology |
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The Wilkinson Microwave Anisotropy Probe (WMAP), originally known as the Microwave Anisotropy Probe(MAP) was a spacecraft operating from 2001 to 2010 which measured differences across the sky in the temperature of the cosmic microwave background (CMB) – the radiant heat remaining from the Big Bang.[3][4] Headed by ProfessorCharles L. Bennett of Johns Hopkins University, the mission was developed in a joint partnership between the NASAGoddard Space Flight Center and Princeton University.[5] The WMAP spacecraft was launched on June 30, 2001 from Florida. The WMAP mission succeeded the COBE space mission and was the second medium-class (MIDEX) spacecraft in the NASA Explorers program. In 2003, MAP was renamed WMAP in honor of cosmologist David Todd Wilkinson(1935–2002),[5] who had been a member of the mission's science team. After 9 years of operations, WMAP was switched off in 2010, following the launch of the more advanced Planck spacecraft by ESA in 2009.
WMAP's measurements played a key role in establishing the current Standard Model of Cosmology: the Lambda-CDM model. The WMAP data are very well fit by a universe that is dominated by dark energy in the form of a cosmological constant. Other cosmological data are also consistent, and together tightly constrain the Model. In the Lambda-CDM model of the universe, the age of the universe is 13.772±0.059 billion years. The WMAP mission's determination of the age of the universe to better than 1% precision was recognized by the Guinness Book of World Records.[6] The current expansion rate of the universe is (see Hubble constant) of 69.32±0.80 km·s−1·Mpc−1. The content of the universe presently consists of 4.628%±0.093% ordinary baryonic matter; 24.02%+0.88%
−0.87% Cold dark matter (CDM) that neither emits nor absorbs light; and 71.35%+0.95%
−0.96% of dark energy in the form of a cosmological constant that accelerates the expansion of the universe.[7] Less than 1% of the current contents of the universe is in neutrinos, but WMAP's measurements have found, for the first time in 2008, that the data prefers the existence of a cosmic neutrino background[8] with an effective number of neutrino species of 3.26±0.35. The contents point to a Euclidean flat geometry, with curvature () of −0.0027+0.0039
−0.0038. The WMAP measurements also support the cosmic inflationparadigm in several ways, including the flatness measurement.
−0.87% Cold dark matter (CDM) that neither emits nor absorbs light; and 71.35%+0.95%
−0.96% of dark energy in the form of a cosmological constant that accelerates the expansion of the universe.[7] Less than 1% of the current contents of the universe is in neutrinos, but WMAP's measurements have found, for the first time in 2008, that the data prefers the existence of a cosmic neutrino background[8] with an effective number of neutrino species of 3.26±0.35. The contents point to a Euclidean flat geometry, with curvature () of −0.0027+0.0039
−0.0038. The WMAP measurements also support the cosmic inflationparadigm in several ways, including the flatness measurement.
The mission has won various awards: according to Science magazine, the WMAP was the Breakthrough of the Year for 2003.[9] This mission's results papers were first and second in the "Super Hot Papers in Science Since 2003" list.[10] Of the all-time most referenced papers in physics and astronomy in the INSPIRE-HEP database, only three have been published since 2000, and all three are WMAP publications. Bennett, Lyman A. Page, Jr., and David N. Spergel, the latter both of Princeton University, shared the 2010 Shaw Prize in astronomy for their work on WMAP.[11] Bennett and the WMAP science team were awarded the 2012 Gruber Prize in cosmology.
As of October 2010, the WMAP spacecraft is derelict in a heliocentric graveyard orbit after 9 years of operations.[12] All WMAP data are released to the public and have been subject to careful scrutiny. The final official data release was thenine-year release in 2012.[13][14]
Some aspects of the data are statistically unusual for the Standard Model of Cosmology. For example, the largest angular-scale measurement, the quadrupole moment, is somewhat smaller than the Model would predict, but this discrepancy is not highly significant.[15] A large cold spot and other features of the data are more statistically significant, and research continues into these.
Thursday, 12 May 2016
Big Bounce
The Big Bounce: The big bang may not have been the beginning of the universe, but merely the beginning of one of an infinite series of universes. Yeah, wrap your mind around that!Courtesy Pat Rawlings/SAICThe Big Bang and the new kid - the Big Bounce - are facing off and it looks as if the Big Bounce is pulling ahead in the polls. Big bounce theory, proposed by Martin Bojowald, is based on loop quantum gravity. And what, you may ask, is loop quantum gravity??
Well, since you asked so nicely...loop quantum gravity - or loop gravity - is a theory of spacetime that attempts to reconcile quantum mechanics and general relativity, according to Wikipedia. Basically, loop gravity tries to prove that gravity is quantized (or broken down into discrete steps). Read more here.
So now that you know a little bit about loop gravity, we can move on to the theory at hand. The big bounce says that the universe is like a bouncy ball. When the ball hits the ground, the universe is at its smallest; as the ball rises above the ground, the universe expands; as the ball moves back towards the ground, the universe begins to implode; when the ball starts to rise after hitting the ground, the universe expands again... You get the idea.
Where the big bounce differs from the big bang is that it resolves the issue of the big bang singularity. And again, you may ask, what in the world is the big bang singularity? Well, for those of you not in the know: the big bang singularity is the single point from which the entire universe is supposed to have sprung. It is, in fact, the major sticking point in the big bang theory; the calculations just can't account for such a singularity.
Well, since you asked so nicely...loop quantum gravity - or loop gravity - is a theory of spacetime that attempts to reconcile quantum mechanics and general relativity, according to Wikipedia. Basically, loop gravity tries to prove that gravity is quantized (or broken down into discrete steps). Read more here.
So now that you know a little bit about loop gravity, we can move on to the theory at hand. The big bounce says that the universe is like a bouncy ball. When the ball hits the ground, the universe is at its smallest; as the ball rises above the ground, the universe expands; as the ball moves back towards the ground, the universe begins to implode; when the ball starts to rise after hitting the ground, the universe expands again... You get the idea.
Where the big bounce differs from the big bang is that it resolves the issue of the big bang singularity. And again, you may ask, what in the world is the big bang singularity? Well, for those of you not in the know: the big bang singularity is the single point from which the entire universe is supposed to have sprung. It is, in fact, the major sticking point in the big bang theory; the calculations just can't account for such a singularity.
So for years, this singularity has been an assumption inherent in the theory. And you know what the problem with assuming is...
This is where the big bounce starts to look mighty good! The big bounce suggests that, as the universe implodes, the energy density of space increases to a point that gravity ceases to be attractive and repulses instead. When gravity becomes repulsive, the universe stops shrinking and begins to expand. Once the density moderates, gravity switches back to being attractive. This explains the explosive expansion seen and accounted for in the big bang theory.Big Bounce: The universe implodes until gravity becomes repulsive and a new universe explodes from the ashes, so to speak.Courtesy Relativity 4 Engineers
Now here is where the big bounce gets really cool! The idea that the universe implodes and explodes like a ball bouncing leads Bojowald to believe that there have been an infinite number of universes before ours and an infinite number of universes to come. Each universe expands, increasing in inertia (or disorder) until it implodes, thus clearing the slate for the new universe.
This is where the big bounce starts to look mighty good! The big bounce suggests that, as the universe implodes, the energy density of space increases to a point that gravity ceases to be attractive and repulses instead. When gravity becomes repulsive, the universe stops shrinking and begins to expand. Once the density moderates, gravity switches back to being attractive. This explains the explosive expansion seen and accounted for in the big bang theory.Big Bounce: The universe implodes until gravity becomes repulsive and a new universe explodes from the ashes, so to speak.Courtesy Relativity 4 Engineers
Now here is where the big bounce gets really cool! The idea that the universe implodes and explodes like a ball bouncing leads Bojowald to believe that there have been an infinite number of universes before ours and an infinite number of universes to come. Each universe expands, increasing in inertia (or disorder) until it implodes, thus clearing the slate for the new universe.
Sunday, 8 May 2016
NASA : Satellites to See Mercury Enter Spotlight on May 9
By NASA
It happens only a little more than once a decade – and the next chance to see it is Monday, May 9. Throughout the U.S., sky watchers can watch Mercury pass between Earth and the sun in a rare astronomical event known as a planetary transit. Mercury will appear as a tiny black dot as it glides in front of the sun’s blazing disk over a period of seven and a half hours. Three NASA satellites will be providing images of the transit and one of them will have a near-live feed.
Although Mercury zooms around the sun every 88 days, Earth, the sun and Mercury rarely align. And because Mercury orbits in a plane that is tilted from Earth’s orbit, it usually moves above or below our line of sight to the sun. As a result, Mercury transits occur only about 13 times a century.
Transits provide a great opportunity to study the way planets and stars move in space – information that has been used throughout the ages to better understand the solar system and which still helps scientists today calibrate their instruments. Three of NASA's solar telescopes will watch the transit for just that reason.
The May 9 Mercury transit will occur between about 7:12 a.m. and 2:42 p.m. EDT. Mercury is too small to see without magnification, but it can be seen with a telescope or binoculars. These must be outfitted with a solar filter as you can't safely look at the sun directly.
“Astronomers get excited when any two things come close to each other in the heavens,” said Louis Mayo, program manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “This is a big deal for us.”
Mercury transits have been key to helping astronomers throughout history: In 1631, astronomers first observed a Mercury transit. Those observations allowed astronomers to measure the apparent size of Mercury’s disk, as well as help them estimate the distance from Earth to the sun.
“Back in 1631, astronomers were only doing visual observations on very small telescopes by today’s standards,” said Mayo.
Since then, technological advancements have allowed us to study the sun and planetary transits in greater detail. In return, transits allow us to test our spacecraft and instruments.
Scientists for the Solar and Heliospheric Observatory, or SOHO (jointly operated by NASA and ESA, the European Space Agency), and NASA’sSolar Dynamics Observatory, or SDO, will work in tandem to study the May 9 transit. The Hinode solar mission will also observe the event. Hinode is a collaboration between the space agencies of Japan, the United States, the United Kingdom and Europe led by the Japan Aerospace Exploration Agency.
SOHO launched in December 1995 with 12 instruments to study the sun from the deep solar core all the way out to the sun's effects on the rest of the solar system. Two of these instruments — the Extreme ultraviolet Imaging Telescope and the Michelson Doppler Imager — will be brought back into full operation to take measurements during the transit after five years of quiescence.
For one thing, the SOHO will measure the sun’s rotation axis using images captured by the spacecraft.
“Instruments on board SDO and SOHO use different spectral lines, different wavelengths and they have slightly different optical properties to study solar oscillations,” said SOHO Project Scientist Joseph Gurman. “Transit measurements will help us better determine the solar rotation axis.”
Such data is another piece of a long line of observations, which together help us understand how the sun changes over hours, days, years and decades.
“It used to be hard to observe transits,” Gurman said. “If you were in a place that had bad weather, for example, you missed your chance and had to wait for the next one. These instruments help us make our observations, despite any earthly obstacles.”
SDO will be able to use the transit to help with instrument alignment. Because scientists know so precisely where Mercury should be in relationship to the sun, they can use it as a marker to fine tune exactly how their instruments should be pointed.
The transit can also be used to help calibrate space instruments. The utter darkness of the planet provides an opportunity to study effects on the observations of stray light within the instrument. The backside of Mercury should appear black as it moves across the face of the sun. But because instruments scatter some light, Mercury will look slightly illuminated.
“It’s like getting a cataract — you see stars or halos around bright lights as though you are looking through a misty windshield,” said SDO Project Scientist Dean Pesnell. “We have the same problem with our instruments.”
Scientists run software on the images to try and mitigate the effect and check whether it can remove all of the scattered light.
For those of us down on the ground, it is worth trying to find a local astronomy club with a solar telescope to see if you can witness this rare event. Alternatively, a near-live feed of SDO images will be available at www.nasa.gov/transit.
Saturday, 7 May 2016
Evolutionary Theory (Part 1)
Evolution is change in the heritable traits of biological populations over successive generations. Evolutionary processes give rise to diversity at every level of biological organisation, including the levels of species, individual organisms, andmolecules.
All life on Earth shares a common ancestor known as the last universal ancestor, which lived approximately 3.5–3.8 billion years ago, although a study in 2015 found "remains of biotic life" from 4.1 billion years ago in ancient rocks inWestern Australia.(by wikipedia).
Brief History of Evolutionary Theory Before Darwin :
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