Indonesia dan Sepotong Kue
(Oleh: Herdi Yustiadi,)
Jika kita berpikir tentang karunia Allah SWT tentulah akan
takjub dan bersyukur. Bayangkan saja seekor cicak yang tidak memiliki sayap, tapi dia bisa
mendapatkan rezeki dari Penciptanya dengan mendatangkan seekor nyamuk atau serangga. Yang perlu dilakukan
oleh cicak itu padahal hanya merayap....menjemput rezekinya.
Sebagai umat Islam kita juga patut bersyukur bagaimana Allah
SWT telah memberikan kekayaan alam yang berlimpah. Di Timur Tengah dengan kekayaan
minyaknya, di Asia Tenggara dengan kekayaan alam minyak, gas alam, mineral, flora dan fauna
baik di darat maupun lautannya.
Semua kekayaan alam tersebut ada di Indonesia Raya tercinta yang
berpenduduk mayoritas muslim ini. Lalu apa yang harus kita lakukan?.... ya “merayaplah”....
jemput rezeki itu. Namun rezeki yang kita miliki itu ternyata sekaligus menjadi
ujian (fitnah) bagi kita, karena banyakbangsa-bangsa lain yang mengaku superior datang silih
berganti memperebutkan kekayaan
Nuswantara ini. Dan... Indonesia seperti layaknya sepotong
kue yang yang diperebutkan. Dahulu kita dirampok dengan orang-orang berwajah bengis dengan bedil dan
meriamnya, namun sekarang dengan orang-orang berwajah ramah dengan mass media nya.
Namun demikian sebagaimana “brutal” nya kekayaan alam kita
dikeruk dan lari ke luar negeri... ada kabar baik.... (?) negara kita masih berdiri dan masih punya
mall-mall mewah...
Sebagai pemilik harta, tentunya kita memiliki pilihan:
menyerahkan harta yang diminta atau menolak/mempertahankannya. Tentu itu suatu pilihan yang
sulit, karena penolakan itu biasanya diikuti oleh ancaman. Seperti layaknya Dajjal, mereka datang
dengan pilihan: air atau api. Namun air hakikatnya api, dan api hakikatnya air. Seolah air itu akan
memberikan kesejukan tetapi ternyata berisi ancaman neraka di dalamnya, begitu sebaliknya dengan
tawaran api yang pada hakikatnya berisi ganjaran surga dibaliknya.
Mengapa air tapi berisi api? Lihat saja tawaran-tawaran yang
mereka lakukan: kemerdakaan, kebebasan dan tatanan ekonomi, sosial dan budaya yang seolah
menyejukkan, tapi membuat kita makin lama menjauh dari fitrah kita untuk selalu ingat akan
Tuhannya dan akhirat, tempat kita berpulang nanti.
Alih-alih daripada pilihan lain (penolakan)
yang dapat menjadi musibah ancaman.... keamanan. Kok mirip preman pasar ya...? Lalu apa saja yang mereka ambil selain SDA? Ternyata
diam-diam mereka juga mengambil pola hidup Islami yang penuh keseimbangan dan keadilan. Satu
contoh diantaranya, lihat saja kasus-kasus korupsi milayaran dan trilyunan yang dilakukan oleh
sekelompok orang tertentu yang dekat dengan sumbu kekuasaan. Karena korupsi itu dianggap sebagai factor
pendorong konsumsi (to consume) lebih dan tentunya berhutang lebih.
Lalu apakah kita akan puas hidup dengan remah-remah kue yang
ada dan akhirnya kita hidup kelaparan di akhirat nanti dengan memakan buah zaqquum
karena cara hidup yang kita lakukan di dunia...? Na’uwdzubillahi min dzalik... Kita jauhkan diri
kita dan keluarga kita dari siksa api neraka.
Rally in Uranium Prices Is Unlikely to Last
Gains Fueled by Ukraine Crisis, Mine Unrest Don't Offset Oversupply
Sept. 14, 2014 4:33 p.m. ET
http://online.wsj.com/articles/rally-in-uranium-prices-is-unlikely-to-last-1410726782
SYDNEY—A multiweek rally in uranium prices fanned by the Ukraine conflict and labor unrest at a large mine in Canada looks
unlikely to continue for long as the reality of oversupply and
lackluster demand sinks in among buyers of the nuclear fuel.
Industry
analysts and some uranium producers believe that even as supplies fall,
a substantial increase in demand is needed to drive prices up to levels
that would make new investments worthwhile, when many operations are
running at a loss.
Uranium prices have surged 15% since the start of August, shaking off a multiyear glut-induced slump.
A gauge of more than 20 commodities, meanwhile, dropped more than 4%.
Uranium now trades at US$32.75 a pound, up from a nine-year low of US$28
in May.
The gain was fueled partly by speculation that Western sanctions against Russia
over its conduct in Ukraine could squeeze supplies. Russia produces
only 5% of the world's uranium but is a leading provider of enrichment
services to many Western utility companies. Prices also surged after
production was interrupted by a labor dispute at
Cameco Corp.'s
CCO.T +2.46%
McArthur River operation, the world's largest uranium mine, in Saskatchewan, Canada.
"Let's not get carried away by the little blip that's happened in the past few weeks,"
Rio Tinto's
RIO.AU -0.16%
energy chief executive,
Harry Kenyon-Slaney,
said at a recent event in Sydney. The market had been so weak for
so long that the 15% lift in prices was of little help to mining
companies, he said.
Demand for uranium ore hasn't recovered since the Fukushima Daiichi disaster.
Bloomberg News
Demand for the fuel hasn't recovered since the disaster at Japan's Fukushima Daiichi nuclear-power plant in 2011, which sparked nuclear-plant closures across the country and tarnished uranium's image globally.
Still,
some analysts are convinced that the uranium market is strengthening
gradually. Macquarie Group Ltd. reckons that an oversupply of almost
12,000 metric tons last year will shrink to 3,200 tons this year.
Reductions
in supply may prevent prices sinking back to their recent lows, but a
sustained recovery could be a way off, according to Macquarie's
Stefan Ljubisavljevic.
It is difficult to see anything but a surplus for the next five
years unless some unprofitable mines close, he said. The only major
facility to have been closed recently was
Paladin Energy Ltd.
PDN.AU -3.57%
's Kayelekera mine in Malawi.
The
biggest producers of the fuel, such as Rio Tinto, aren't betting on a
quick recovery but remain upbeat about uranium's longer-term outlook as
countries such as China and India bring new reactors online.
Macquarie,
which anticipates a 6% drop in output from uranium mines this year,
estimates that around half the industry could be unprofitable at current
prices.
"The industry is going through
some very tough times, but at some point, new production will have to be
incentivized to deliver into the power programs, particularly in
China," said Rio Tinto's Mr. Kenyon-Slaney.
China has stepped up efforts to introduce cleaner energy and has the world's largest pipeline of nuclear-power plants.
Australia recently struck a deal for its mining companies to sell uranium for use in India.
Japan's
nuclear watchdog this month said two reactors at the Sendai plant on
the southern island of Kyushu had met stricter guidelines imposed after
the Fukushima accident—putting them first in line among the country's 48
idled reactors to be restarted. But antinuclear sentiment after the
disaster means it is unclear when the reactors might return to service.
Meanwhile,
state governments in resource-rich Australia have been encouraging the
growth of the nation's uranium industry. A decadeslong ban on uranium
production in Queensland was lifted in July, opening the door to new
applications to build mines in the state. The government of New South
Wales this month said it would invite six companies to apply for
exploration licenses.
Still, there is
expected to be little investment in new projects until the market stages
a more substantial comeback. Cameco said it would need to see much
higher uranium prices before it started construction of its proposed
Kintyre uranium mine in Western Australia.
"The
nuclear industry is still in the midst of upheaval," said
Jonathan Hinze,
senior vice president at nuclear-research firm Ux Consulting Co.
But he said there was some hope for the industry, given decreased
willingness among traders and producers to undercut each other's prices
to win customers.
Write to Rhiannon Hoyle at rhiannon.hoyle@wsj.com
http://online.wsj.com/articles/rally-in-uranium-prices-is-unlikely-to-last-1410726782
Top Sources of Powerful Space Radiation Are Shockers
by Charles Q. Choi, SPACE.com Contributor | December 01, 2011 07:12am ET
This all-sky image,
constructed from two years of observations by NASA's Fermi Gamma-ray
Space Telescope, shows how the sky appears in gamma-ray light. Brighter
colors indicate brighter gamma-ray sources. A diffuse glow fills the sky
and is brightest along the plane of our galaxy (middle). Discrete
gamma-ray sources include pulsars and supernova remnants within our
galaxy as well as distant galaxies powered by supermassive black holes.
New maps of gamma-ray light streaming in from the sky reveal some surprising sources of this highest-energy form of light, including objects that were never detected before.
NASA's Fermi Gamma-Ray Space Telescope, orbiting around Earth, scans the entire sky every three hours. It watches for not only continuous sources of this dangerous radiation but numerous sudden explosions, such as gamma-ray bursts in the distant universe and flares from the sun.
The latest maps produced by the satellite's Large Area Telescope (LAT) identified 1,873 cosmic gamma-ray sources. Although more than half of these astronomical objects are the usual suspects — active galaxies, whose supermassive central black holes spew forth radiation as they rip apart the matter falling into them — more than a third of them were never seen in any other wavelength of light, visible or otherwise.
To highlight the range of gamma-ray sources in this new census, the Fermi team created a "Top 10" list. Five of the 10 "top" gamma-ray sources are within the Milky Way. [Top 10 Strangest Things in Space]
Within our galaxy
One enigma inside the Milky Way has the cumbersome designation 2FGL J0359.5+5410. It resides in the constellation Camelopardalis, near the populous midplane of our galaxy.
"2FGL J0359.5+5410 might belong to a new class of object not detected before in the gamma-ray band," Tosti told SPACE.com.
Meanwhile, W44 is a 20,000-year-old object about 9,800 light-years away in the constellation Aquila. Researchers think W44 is the wreckage of a supernova, an exploded star. Fermi's observations of W44 strongly hint that gamma-rays are coming from where the supernova remnant's expanding shock wave interacts with cold, dense gas clouds – perhaps emerging from speedy protons colliding with gas atoms.
Fermi's LAT mapped GeV-gamma-ray emission (magenta)
from the W44 supernova remnant. The features clearly align with
filaments detectable in other wavelengths. This composite merges X-rays
(blue) from the Germany-led ROSAT mission, infrared (red) from NASA's
Spitzer Space Telescope, and radio (orange) from the NRAO's Very Large
Array near Socorro, N.M.
Credit: NASA/DOE/Fermi LAT Collaboration, ROSAT, JPL-Caltech, and NRAO/AUI
Credit: NASA/DOE/Fermi LAT Collaboration, ROSAT, JPL-Caltech, and NRAO/AUI
Crab nebula
Another supernova remnant source of gamma-rays is the famous Crab Nebula. Located 6,500 light-years away in the constellation Taurus, the nebula is left over from a supernova whose light reached Earth in 1054. At the heart of an expanding gas cloud around what is left of the original star's core is a pulsar spinning 30 times a second.
Fermi and the Italian Space Agency's AGILE satellite have detected a number of short-lived gamma-ray flares at energies hundreds of times higher than the nebula's observed X-ray variations. The researchers suggest these "superflares" are due to electrons near the pulsar, accelerated to energies a thousand trillion times greater than that of visible light — far beyond what can be achieved by the Large Hadron Collider near Geneva, Switzerland, now the most powerful particle accelerator on Earth.
In addition to supernovas and their remnants, regular novas can emit gamma-rays.
V407 Cygni is a binary star system about 9,000 light-years away in the constellation Cygnus that contains a compact white dwarf and a red giant star about 500 times the size of the sun.
This system occasionally flares with outbursts known as novas, when gas from the red giant collects onto the white dwarf's surface and eventually explodes. Gamma-rays from these novas defied expectations — scientists had not expected such explosions to have enough power to generate high-energy gamma rays.
Pulsars make up about 6 percent of Fermi's new map of gamma-ray sources. Working together with radio astronomers, the Fermi team found that pulsar PSR J0101-6422 in the southern constellation of Tucana pulses with gamma-rays nearly 400 times a second, matching up with radio data.
Beyond the Milky Way
One source close to home is the Andromeda Galaxy (M31), which at a distance of 2.5 million light-years is the nearest spiral galaxy, one of similar size and structure as our own Milky Way. The gamma-rays seen from M31 are mostly caused by high-energy cosmic rays slamming into the gas between the stars.
"It took two years of LAT observations to detect M31," said study coauthor Jürgen Knödlseder at the Research Institute for Astrophysics and Planetology in Toulouse, France. "We concluded that the Andromeda Galaxy has fewer cosmic rays than our own Milky Way, probably because M31 forms stars — including those that die as supernovae, which help produce cosmic rays — more slowly than our galaxy."
The cores of active galaxies spray out jets of particles at near-light speed, and such galaxies are called blazars when these jets point our way. PKS 0537-286is a variable blazar, whose jet can vary in brightness over time by more than a hundredfold. This object is so far away, we are viewing it as it was when the universe was just 2 billion years old. "The general picture is that the variability is due to the formation of perturbations or instabilities in the jet," Tosti explained.
The center of the Cigar Galaxy (M82) is bright for another reason. Located 12 million light-years away in the constellation Ursa Major, this is a so-called starburst galaxy, whose core forms 10 times more young stars than the Milky Way does. This hyperactivity guarantees a high rate of supernovas, as most of the short-lived stars come to explosive ends bright in gamma-rays.
Beyond the core
Gamma-rays are not just limited to galactic cores, as can be seen with the giant elliptical galaxy Centaurus A, also known as NGC 5128, which is located 12 million light-years away in the southern constellation Centaurus. The galaxy is bright with radio waves, emitted from million-light-year-wide lobes of gas hurled out by the supermassive black hole at the galaxy's center. Fermi detected high-energy gamma rays from these lobes as well. The radio emissions come from fast-moving particles, which can slam into photons and boost them into gamma-ray levels, researchers said.
One mystery object is 2FGL J1305.0+1152, located in the constellation Virgo and high above our galaxy's midplane. Its gamma-ray spectrum — the relative amounts of different energies of gamma-rays — resembles neither a pulsar nor a blazar.
Tosti did note this enigma is located in a region where gamma-ray sources are mostly active galactic nuclei, the bright centers of galaxies with hungry supermassive black holes. "Its probability to be an active galactic nucleus might be high, but not 100 percent," he said. Only with the discovery of a counterpart of this source at other wavelengths will we be able to disclose its mystery, he added.
"I would say that the work is just starting," Tosti said. "We were able to detect the sources — now we have to understand better the physical mechanisms that are responsible of their emissions."
Gamma-ray sources aren't the only mysteries that Fermi stands to unravel. Its observations are providing astrophysicists with hope of solving the old puzzle of the origin of cosmic rays.
"Fermi and other multi-wavelength studies are providing growing evidence that supernova remnants are the source of the bulk of galactic cosmic rays," Tosti said.
"However, the sample of supernova remnants observed by Fermi is still too small to declare the problem solved. I feel that this longstanding mystery will be solved soon — it would be nice if this could happen next year, when there will be the celebration of the centenary of the discovery of cosmic rays by Hess in 1912."
Tosti and his colleagues detailed their findings Sept. 9 at a meeting of the American Astronomical Society's High Energy Astrophysics Division in Newport, R.I.
Follow SPACE.com for the latest in space science and exploration news on Twitter @Spacedotcom and on Facebook.
Tidak ada komentar:
Posting Komentar