Category: Photography

  • Backwards Black Holes Might Make Bigger Jets

    PASADENA, Calif. – Going against the grain may turn out to be a powerful move for black holes. New research suggests supermassive black holes that spin backwards might produce more ferocious jets of gas. The results have broad implications for how galaxies change over time.

    “A lot of what happens in an entire galaxy depends on what’s going on in the miniscule central region where the black hole lies,” said theoretical astrophysicist David Garofalo of NASA’s Jet Propulsion Laboratory in Pasadena, Calif. Garofalo is lead author of a new paper that appeared online May 27 in the Monthly Notices of the Royal Astronomical Society. Other authors are Daniel A. Evans of the Massachusetts Institute of Technology, Cambridge, Mass., and Rita M. Sambruna of NASA Goddard Space Flight Center, Greenbelt, Md.

    Black holes are immense distortions of space and time with gravity that is so great, even light itself cannot escape. Astronomers have known for more than a decade that all galaxies, including our own Milky Way, are anchored by tremendous, so-called supermassive black holes, containing billions of suns’ worth of mass. The black holes are surrounded and nourished by disks of gas and dust, called accretion disks. Powerful jets stream out from below and above the disks like lasers, and fierce winds blow off from the disks themselves.

    The black holes can spin either in the same direction as the disks, called prograde black holes, or against the flow – the retrograde black holes. For decades, astronomers thought that the faster the spin of the black hole, the more powerful the jet. But there were problems with this “spin paradigm” model. For example, some prograde black holes had been found with no jets.

    Garofalo and his colleagues have been busy flipping the model on its head. In previous papers, they proposed that the backward, or retrograde, black holes spew the most powerful jets, while the prograde black holes have weaker or no jets.

    The new study links the researchers’ theory with observations of galaxies across time, or at varying distances from Earth. They looked at both “radio-loud” galaxies with jets, and “radio-quiet” ones with weak or no jets. The term “radio” comes from the fact that these particular jets shoot out beams of light mostly in the form of radio waves.

    The results showed that more distant radio-loud galaxies are powered by retrograde black holes, while relatively closer radio-quiet objects have prograde black holes. According to the team, the supermassive black holes evolve over time from a retrograde to a prograde state.

    “This new model also solves a paradox in the old spin paradigm,” said David Meier, a theoretical astrophysicist at JPL not involved in the study. “Everything now fits nicely into place.”

    The scientists say that the backward black holes shoot more powerful jets because there’s more space between the black hole and the inner edge of the orbiting disk. This gap provides more room for the build-up of magnetic fields, which fuel the jets, an idea known as the Reynold’s conjecture after the theoretical astrophysicist Chris Reynolds of the University of Maryland, College Park.

    “If you picture yourself trying to get closer to a fan, you can imagine that moving in the same rotational direction as the fan would make things easier,” said Garofalo. “The same principle applies to these black holes. The material orbiting around them in a disk will get closer to the ones that are spinning in the same direction versus the ones spinning the opposite way.”

    Jets and winds play key roles in shaping the fate of galaxies. Some research shows that jets can slow and even prevent the formation of stars not just in a host galaxy itself, but also in other nearby galaxies.

    “Jets transport huge amounts of energy to the outskirts of galaxies, displace large volumes of the intergalactic gas, and act as feedback agents between the galaxy’s very center and the large-scale environment,” said Sambruna. “Understanding their origin is of paramount interest in modern astrophysics.”

    The California Institute of Technology, Pasadena, manages JPL for NASA.

    Posted via web from Monicks: Unleashed

  • Aggressive Waves Photography

    This post is dedicated to Waves and Surfing Waves Photography. Waves booming against the seashore can be a very soothing experience for anyone. Almost everyone loves the beauty of sea and ocean waves are the most attractive and appealing thing for everyone. However, waves do not have to look calm and nice. They can be aggressive, too.

    Ocean wave photos, pictures of wave curls, ocean wave pictures, and other big wave pictures will bring the ocean to you. Here are some amazing examples for your inspiration. Hope that you like them — and don’t forget to share your comments!

    Waves and Surf Photography

    Cory Scott

    Waves 42 in 40 Aggressive Examples of Waves Photography

    Jeff Divine

    Waves 3 in 40 Aggressive Examples of Waves Photography

    One Sequence, Eight Pros

    Waves 39 in 40 Aggressive Examples of Waves Photography

    Gold Coast

    Waves 34 in 40 Aggressive Examples of Waves Photography

    Awesome Waves

    Waves 4 in 40 Aggressive Examples of Waves Photography

    Raku Art

    Waves 29 in 40 Aggressive Examples of Waves Photography

    Jeff Divin

    Waves 5 in 40 Aggressive Examples of Waves Photography

    Sandy Shack

    Waves 26 in 40 Aggressive Examples of Waves Photography

    Waves

    Waves 7 in 40 Aggressive Examples of Waves Photography

    Sunshine

    Waves 27 in 40 Aggressive Examples of Waves Photography

    Wave Surf

    Waves 8 in 40 Aggressive Examples of Waves Photography

    Wave Surf

    Waves 9 in 40 Aggressive Examples of Waves Photography

    Triple Crown

    Waves 28 in 40 Aggressive Examples of Waves Photography

    Wave Surfing

    Waves 10 in 40 Aggressive Examples of Waves Photography

    Waves

    Waves 11 in 40 Aggressive Examples of Waves Photography

    Waves Surfing

    Waves 12 in 40 Aggressive Examples of Waves Photography

    Waves

    Waves 13 in 40 Aggressive Examples of Waves Photography

    Two Crests

    Waves 15 in 40 Aggressive Examples of Waves Photography

    Seascape Distilled: Wave Panning

    Waves 16 in 40 Aggressive Examples of Waves Photography

    Wave Surf

    Waves 17 in 40 Aggressive Examples of Waves Photography

    Gold Nugget

    Waves 33 in 40 Aggressive Examples of Waves Photography

    Flashlight

    Waves 32 in 40 Aggressive Examples of Waves Photography

    Wave Buzzard

    Waves 18 in 40 Aggressive Examples of Waves Photography

    Sand & Sea ~ Curtin Wave

    Waves 19 in 40 Aggressive Examples of Waves Photography

    Pacific waves

    Waves 20 in 40 Aggressive Examples of Waves Photography

    Catch A Wave

    Waves 21 in 40 Aggressive Examples of Waves Photography

    wave crash

    Waves 22 in 40 Aggressive Examples of Waves Photography

    Cabo – Waves

    Waves 46 in 40 Aggressive Examples of Waves Photography

    Mountain Waves

    Waves 35 in 40 Aggressive Examples of Waves Photography

    Huge Waves

    Waves 36 in 40 Aggressive Examples of Waves Photography

    NZ’S SUPER SHOOTER

    Waves 37 in 40 Aggressive Examples of Waves Photography

    ONE SEQUENCE, EIGHT PROS

    Waves 40 in 40 Aggressive Examples of Waves Photography

    JOSH KERR: “IT FELT LIKE MY LEG HAD SPLIT IN HALF!”

    Waves 41 in 40 Aggressive Examples of Waves Photography

    CORY SCOTT

    Waves 43 in 40 Aggressive Examples of Waves Photography

    Posted via web from Monicks: Unleashed

  • Astrophotography | Comet C/2009 R1 (McNaught) in Andromeda

    Comet C/2009 R1 (McNaught) in Andromeda
    Image Details Imaging Details
    Comet: 
    C/2009 R1 (McNaught)

    Discoverer: 
    Robert McNaught 
    Sep 09, 2009

    Type: 
    Hyperbolic

    Period: 
    N/A

    Constellation: 
    Andromeda

    RA / Dec: 
    02h 21m 36s / 
    42° 05′ 32″

    Distance: 
    175.1 million km

    Magnitude: 
    5.0 – 6.0

    Date: 
    June 8, 2010 
    03:15 – 04:07 UT+3

    Location: 
    Athens, Greece 
    (38.2997° N, 23.7430° E)

    Equipment: 
    AP 160/f7.5 StarFire EDF
    AP 1200GTO GEM 
    SBIG ST-10XME 
    SBIG CFW10 
    SBIG LRGB filters

    Integrations:

    Lum :  10 min (10 x 1 min)
    Red :  10 min (10 x 1 min)
    Green :  10 min (10 x 1 min)
    Blue :  10 min (10 x 1 min)
    Binning :  1×1 (Lum), 1×1 (RGB)

    Image Scale: 
    1.17″ / pixel

    Temperatures:

    Ambient : + 19.0 ° C
    CCD Chip : – 17.5 ° C

    Software: 
    CCDSoft V5.00.195
    CCDStack V1.6.0.5
    Photoshop CS2

    These travelling masses of ice and dust galloping throughout the universe are believed to have shaped the course of life on this planet. As a result of comet-hunting, many deep-sky objects including nebulae and galaxies have been discovered with perhaps the most obvious collection being the 109 (or 110) DSO’s attributed to Charles Messier. With over 1000 comets now having been catalogued and approximately 200 having been established as being periodic, historical records suggest comets to have been observed and documented as far back as 240 BC (Comet Halley by the Chinese).

    Comets are appealing to amateurs for a variety of reasons: they lead to incredible photographs thanks to their glowing and colourful tails extending millions of kilometers as they approach the sun and the ice and various frozen gases in the nucleus begin to vaporize; they are the precursors of meteor showers as remnants left behind on prior visits are encountered by our planet while we orbit the sun; and they represent an active adventure and form the basis of a “culture” (comet hunters) based on the discovery of new comets during the early dawn hours on the eastern horizon or just after sunset on the western horizon.

    Note: Comet C/2009 R1 (McNaught) illustrated below while passing through the constellation of Andromenda and within the immediate vicinity of the edge-on galaxy NGC 891 was discovered on Sept 9, 2009 by Siding Spring Observatory astronomer Robert McNaught in five plates and was estimated to be magnitude 17.3 to 17.5. Continuous monitoring has revealed a continuing brightening of the nucleus and which is now expected to reach mag 2 by the end of June and early parts of July when it will finally be lost in the morning twilight. Perihelion has been estimated to be July 2, 2010.

    For an ephemeris and orbital elements on this hyperbolic comet from Harvard’s Minor Planet Center, click here. For a simulation of the comet including various orbital elements and physical parameters, click here.

    Note: The comet was only 12 to 19 degrees above the horizon during the imaging session!

     

    via perseus.gr

     

     

    Posted via web from Monicks: Unleashed