Combining high resolution images and infrared spectra collected during the probe's approach, a team of nearly two dozen scientists pinpointed three patches of
water ice on the surface of the comet's «upper» half.
In 2008, however, Andrew Rivkin of Johns Hopkins University in Laurel, Maryland, and Joshua Emery of the SETI Institute in Mountain View, California, found hints (pdf) that the asteroid 24 Themis, which sits in the main asteroid belt between Mars and Jupiter, could have
water ice on its surface.
«Quaoar, a large body in the Kuiper Belt, has crystalline
water ice on its surface, yet conditions there should favour amorphous ice.»
TRAPPIST - 1f, g and h seem to have thin atmospheres and could potentially harbor
water ice on the surface.
Not exact matches
The new system could potentially supply the power human crews
on the Martian
surface would need to energize habitats and run processing equipment to transform resources such as
ice on the planet into oxygen,
water and fuel, NASA said.
but today,
on the
surface, the
water and
ice will kill you fast.
1) Mix flour, butter and
icing sugar in a bowl using two knives to cut the butter until the mixture resembles fine breadcrumbs 2) Add in the egg yolks and vanilla extracts and mix well, then add
iced water until the dough starts to come together 3) Shape the dough into a ball
on a cool, flat, floured
surface 4) Flatten dough into a disc and then wrap in plastic wrap, and chill in the refrigerator for at least 30 minutes 5) Meanwhile, peel, core and slice the apples into as thin slices as possible 6) Mix sugar and ground cinnamon powder with sliced apples and let it rest for a while 7) Pre-heat oven to 180 deg cel 8) Once dough has chilled, roll pastry dough
on a sheet of parchment paper until it has expanded to the size of the tart mold (I used a rough mold the size of a large pizza) 9) Leaving at least an inch of dough free, arrange apple slices by overlapping them slightly in the shape of a circle, starting from the outermost part of the circle, until you reach the inside 10) Fold the edges of dough over the filling and then sprinkle the dough with a bit of sugar 11) Bake for about 40 - 45 minutes, or until the crust is golden brown and the apples are soft 12) Serve warm, with a side of whipped cream or
ice cream (optional)
Then, just as the
surface gets too bad, out comes a bucket brigade;
water on the
ice supposedly lessens the friction.
A cubic yard of air contains hundreds of thousands of microscopic specks, but only about one in a million possesses the exact molecular geometry that will organize
water molecules
on its
surface to spawn an
ice crystal.
A little mineral crystal can act as a template, coaxing
water molecules
on its
surface to organize into the hexagonal lattice of an
ice crystal.
In areas that are both bright and cold,
water ice may be present
on the
surface as frost.
The density of the mammoth main - belt asteroid Ceres suggests it contains a large amount of
water ice, but no clear - cut sign of
ice has been found
on its
surface.
Water ice is present
on the
surface of Comet Tempel 1, suggest observations from NASA's Deep Impact mission.
On the nanometer scale, we observed the coexistence of ordered
surface water and crystallite - like
ice structures, evident in the superposition of Bragg spots and Debye - Scherrer rings.
The new observations suggest
water ice, mixed with organic molecules, is «widespread
on the
surface of the asteroid», Humberto Campins of the University of Central Florida in Orlando reported at a meeting of the American Astronomical Society's Division of Planetary Sciences in Fajardo, Puerto Rico, last week.
Today the small amount of
water detected
on the planet is locked in the polar
ice caps, but recently discovered geological features suggest liquid
water once flowed
on its
surface.
Alice also documented a surprising lack of exposed
water ice on the comet's
surface and identified an extremely volatile, unexpected gas in the comet's atmosphere — molecular oxygen.
«We are in awe that an animal that spends most of its time
on the
surface of sea
ice could swim constantly for so long in
water so cold.»
On Pluto, a slurry of nitrogen and
water ice melted by subsurface heat stands in for lava, the team suggests, freezing solid once it is exposed at the
surface.
Another explanation is cryovolcanism, in which
ice and
water are forced out of the
surface by processes similar to those that drive magma volcanoes
on Earth.
In 2005, NASA's Cassini spacecraft spied jets of
water ice and vapor erupting into space from fissures
on Enceladus, evidence of a salty ocean beneath the saturnian moon's placid icy
surface.
(Size will depend
on the size of your bowl and the size of your
ice cubes — they will need to be big enough for of them to hold two
ice cubes
on its
surface and for both of them to stick out of the
water.)
Even though density measurements suggest that Ceres is roughly one third
water by weight,
water ice should rapidly sublimate away into space
on the dwarf planet's airless, sun - soaked
surface, so its absence at first would seem to be no surprise.
Last year the Herschel Space Observatory detected wisps of
water vapor around the dwarf planet, and since its arrival at Ceres, Dawn has imaged oodles of highly reflective bright spots
on the Cereian
surface that may be sites of exposed
water ice.
According to recent calculations, the upper limit
on the present amount of
water on the Martian
surface is 800,000 to 1.2 million cubic miles, or about 1.5 times the amount of
ice covering Greenland.
During its five - plus months
on the Red Planet, the robot verified the presence of
ice water below the Martian
surface (the Mars Odyssey orbiter first spotted
water there in 2002).
While that
water could initially come from Earth, it could later come from
water ice frozen
on asteroids, in shadowed regions of the moon's
surface, from possible sources
on Mars» two moons, or from Mars itself.
These planets in the habitable zones of their stars, while able to support liquid
water on their
surfaces, develop in dry environments and need to have
ice sent in from farther out.
But last year, Arrigo and his team noted a proliferation of pools of
water, known as melt ponds,
on the
surface of the Chukchi Sea
ice, which were also a few meters thinner than in past years.
Untersee is a good model for Mars, he says, because it is supplied by subglacial melt —
water that accumulates at the bottom of an
ice pile — rather than from
surface melting, which does not occur
on Mars.
But the
water's source — whether melting
ice, rainfall, or groundwater — and its duration
on the
surface are still open questions.
Using spectral readings from telescopes at the Keck Observatory in Hawaii, Hand has found high levels of oxidative chemicals such as sulfate, oxygen, sulfur dioxide and hydrogen peroxide
on Europa's
surface, which are produced as ionizing radiation from Jupiter scours it, splitting apart
water molecules and sulfur compounds in the uppermost layers of its
ice.
Rime forms when droplets of
water vapor deposit directly as
ice on surfaces.
A protein
on the cell
surface of P. syringae binds
water in a way that mimics the structure of an
ice crystal, and this helps start the transformation of cold
water into
ice.
Titan has diverse, carbon - rich chemistry
on a
surface dominated by
water ice, as well as an interior ocean.
It's unclear whether this year's strong El Niño event, which is a naturally occurring phenomenon that typically occurs every two to seven years where the
surface water of the eastern equatorial Pacific Ocean warms, has had any impact
on the Arctic sea
ice minimum extent.
Astronomers have known about Europa's biological trifecta for almost two decades, yet there have always been doubts: For Europa to support life, the vital molecules
on the
surface need to mix with the
water and energy below, and there is a giant slab of
ice lying in between.
There is probably
water -
ice at depth
on Pluto, but the
surface ice is a mixture of frozen methane, ethane, carbon monoxide and nitrogen.
New research shows how a layer of
water on the
surface of
ice — even at temperatures well below freezing — can influence everything from the slipperiness of a skating rink to the electrification of thunderclouds
Water droplets have a tough time gaining purchase
on the roughed - up
surface, boosting its ability to resist
ice formation fourfold over that of «naked» aluminium.
The study marks the first time that human influence
on the climate has been demonstrated in the
water cycle, and outside the bounds of typical physical responses such as warming deep ocean and sea
surface temperatures or diminishing sea
ice and snow cover extent.
Signs of repeated
ice - and snow - melt in a mid-latitude gully may point to the most recent
water activity
on the Red Planet's
surface
The craft is designed to dig into the cementlike layer of
ice that researchers believe lies buried a few inches below the
surface in the planet's polar regions, scanning for signs of past liquid
water and organic compounds, the carbon - rich molecules that make life
on Earth possible.
They found, as expected, that one part of an InaZ protein
on the bacteria's
surface arranges
water molecules into an orderly formation — getting them prepped to form
ice.
In 2005, while exploring the Saturn system, the Cassini spacecraft made a startling discovery: Cryovolcanoes
on Enceladus were spewing jets of
water vapor and
ice into space, possibly from a liquid
water source beneath the
surface.
Beneath the hydrocarbon seas
on the
surface, under a shell of
water ice, lies salty liquid
water.
The research shows that volcanic eruptions beneath a glacial
ice sheet would have created substantial amounts of liquid
water on Mars's
surface around 210 million years ago.
In addition to
water, organic molecules, which could have been deposited
on the
surface by crashing comets, somehow would have to get through the thick shells of
ice for life to form, a situation that puts Saturn's geyser - spewing moon Enceladus at the top of Nimmo's list of potential spots for life.
It is theorized that the process may be similar to what happens
on comets, when
water vapor lifts tiny particles of dust and
ice off the
surface.
Most of the images from Rosetta have been in black & white, so these colour ones are a nice change and show incredible detail, including patches of
water ice on the rocky
surface.