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Saturday, August 6, 2011

USCG Licensing class schedule for Fall 2011

Fall 2011 Schedule for
Zenith Maritime Academy courses
at Windworks Sailing Center

These courses are approved by the USCG for the licensing of US Merchant Mariners. They are linked from the Windworks website as Seattle Merchant Mariner Training.

All Zenith classes run M-F 0900-1700, with a 1-hour lunch break. Half days and 4-hour classes run from 0900 to 1300.


56 hour Operator of Uninspected Passenger Vessel (“Six Pack”) Sep 6 – Sep 16 $800
24 hour OUPV to Master 100 Ton Upgrade Sep 19 – Sep 23 $375
4 hour Auxiliary Sail Endorsement Sep 26 $75
4 hour Commercial Assistance Towing Sep 28 $75

56 hour Operator of Uninspected Passenger Vessel (“Six Pack”) Oct 3 – Oct 14 $800

56 hour Operator of Uninspected Passenger Vessel (“Six Pack”) Nov 7 – Nov 18 $800
4 hour Auxiliary Sail Endorsement Nov 21 $75
4 hour Commercial Assistance Towing Nov 22 $75
56 hour Operator of Uninspected Passenger Vessel (“Six Pack”) Nov 28 – Dec 9 $800
24 hour OUPV to M100 Upgrade Dec 12 – Dec 16 $375
32 hour M100 to M200 Upgrade Dec 19 – Dec 23 $375


For registration contact:

Windworks Sailing Center

7001 Seaview Ave NW Suite 110
Seattle WA 98117
206-784-9386, fax 206-784-2995
www.windworkssailing.com
greg@sail1.com.

Thursday, August 4, 2011

Waterfalls on Barsoom

NASA today released photos of what is very likely brine flowing, in not insignificant amounts, down the side of an equatorial crater on Mars.

From the standpoint of human outmigration and colonization, this isn't exactly a game-changer. We've known for a while that there is a large amount of frozen water at or near the surface of Mars. We've also known for a while that Mars has equatorial surface temperatures as high as 27°C (81°F, which here in Seattle is referred to as a heat-wave), albeit only for a few centimeters above the ground. So it would probably be more unusual if these did not result in Mars having occasional surface water. With a surface atmospheric pressure of some 6 millibars (compared to Earth's average of 1013 mb) we wouldn't expect any surface water to last very long, and the fact that the "surface" water detected appears to be actually embedded in sand or dust is pretty much what we should expect. But for human colonists, this water would not be very much easier (and possibly rather more difficult) to extract and utilize than the near-surface ice which is much more abundant.

On the other hand, from the standpoint of exobiology, this is huge. Because it means that we are officially no longer just searching for fossils of Martian life. It is now genuinely reasonable to imagine that we will find life there, at least in microbial form. Not on the Martian surface, where cosmic and solar radiation would almost certainly sterilize anything possessing anything resembling RNA or DNA. But in the sub-martian aquifers which are necessarily feeding these springs, life may well have survived from a time when Mars was far more hospitable to life as it exists on Earth.

In the search for life on Mars, we now have a definitive starting point.


NASA Spacecraft Data Suggest Water Flowing on Mars

PASADENA, Calif. -- Observations from NASA's Mars Reconnaissance Orbiter have revealed possible flowing water during the warmest months on Mars.

"NASA's Mars Exploration Program keeps bringing us closer to determining whether the Red Planet could harbor life in some form,” NASA Administrator Charles Bolden said, “and it reaffirms Mars as an important future destination for human exploration."

Dark, finger-like features appear and extend down some Martian slopes during late spring through summer, fade in winter, and return during the next spring. Repeated observations have tracked the seasonal changes in these recurring features on several steep slopes in the middle latitudes of Mars' southern hemisphere.

"The best explanation for these observations so far is the flow of briny water," said Alfred McEwen of the University of Arizona, Tucson. McEwen is the principal investigator for the orbiter's High Resolution Imaging Science Experiment (HiRISE) and lead author of a report about the recurring flows published in Thursday's edition of the journal Science.

Some aspects of the observations still puzzle researchers, but flows of liquid brine fit the features' characteristics better than alternate hypotheses. Saltiness lowers the freezing temperature of water. Sites with active flows get warm enough, even in the shallow subsurface, to sustain liquid water that is about as salty as Earth's oceans, while pure water would freeze at the observed temperatures.

"These dark lineations are different from other types of features on Martian slopes," said Mars Reconnaissance Orbiter Project Scientist Richard Zurek of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Repeated observations show they extend ever farther downhill with time during the warm season."

The features imaged are only about 0.5 to 5 yards or meters wide, with lengths up to hundreds of yards. The width is much narrower than previously reported gullies on Martian slopes. However, some of those locations display more than 1,000 individual flows. Also, while gullies are abundant on cold, pole-facing slopes, these dark flows are on warmer, equator-facing slopes.

The images show flows lengthen and darken on rocky equator-facing slopes from late spring to early fall. The seasonality, latitude distribution and brightness changes suggest a volatile material is involved, but there is no direct detection of one. The settings are too warm for carbon-dioxide frost and, at some sites, too cold for pure water. This suggests the action of brines, which have lower freezing points. Salt deposits over much of Mars indicate brines were abundant in Mars' past. These recent observations suggest brines still may form near the surface today in limited times and places.

When researchers checked flow-marked slopes with the orbiter's Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), no sign of water appeared. The features may quickly dry on the surface or could be shallow subsurface flows.

"The flows are not dark because of being wet," McEwen said. "They are dark for some other reason."

A flow initiated by briny water could rearrange grains or change surface roughness in a way that darkens the appearance. How the features brighten again when temperatures drop is harder to explain.

"It's a mystery now, but I think it's a solvable mystery with further observations and laboratory experiments," McEwen said.

These results are the closest scientists have come to finding evidence of liquid water on the planet's surface today. Frozen water, however has been detected near the surface in many middle to high-latitude regions. Fresh-looking gullies suggest slope movements in geologically recent times, perhaps aided by water. Purported droplets of brine also appeared on struts of the Phoenix Mars Lander. If further study of the recurring dark flows supports evidence of brines, these could be the first known Martian locations with liquid water.