Apparently, fewer people visit here....

[Mikey]

Bit of a cock-up on the catering front

Someones eaten all the biscuits

[gr8gonzo]

It could be worse!

[catherine]

*puts hand up*

I'm still here!

[Againesis]

Guilty as charged m'lud.  Not quite as often as I used to be but... :oops:

[Trapezium Artist]

Present and correct, sah!

[Fogeyspasm]

Back from excess amounts of work!

[Brom]

I still keep a washing brief.  

[Mooncat]

I always keep washing my briefs, I'd hate to get run over by a bus and be found to be wearing dirty underpants  

[rogerg]

I always keep washing my briefs, I'd hate to get run over by a bus and be found to be wearing dirty underpants  

heh

[gr8gonzo]

I can imagine the inaccuracies of the obituary:

"He was a big fan of Staind. His favourite biscuit - Fudge Stripes..."

Better safe than sorry.

[Mikey]

I can imagine the inaccuracies of the obituary:

"He was a big fan of Staind.

Not forgetting The Skids

[Mouse]

Never mind all that! Did you know that the most conspicuous feature of Martian surface geology is a sharp contrast, known as the Martian dichotomy, between the rugged southern highlands and the relatively smooth northern basins? The two hemispheres differ in elevation by 1 to 3 km. The average thickness of the Martian crust is 45 km, with 32 km in the northern lowlands region, and 58 km in the southern highlands.

The boundary between the two regions is quite complex in places. One distinctive type of topography is called fretted terrain. It contains mesas, knobs, and flat-floored valleys having walls about a mile high. Around many of the mesas and knobs are lobate debris aprons that have been shown to be rock-covered glaciers.

Many large river valleys cut through the dichotomy.

The Martian dichotomy boundary includes the regions called Deuteronilus Mensae, Protonilus Mensae, and Nilosyrtis Mensae. All three regions have been studied extensively because they contain landforms believed to have been produced by the movement of ice.

The northern lowlands comprise about one-third of the surface of Mars and are relatively flat, with occasional impact craters. The other two-thirds of the Martian surface are the highlands of the southern hemisphere. The difference in elevation between the hemispheres is dramatic. Because of the density of impact craters, scientists believe the southern hemisphere to be far older than the northern plains. The heavily cratered southern highlands date back to the period of heavy bombardment. Three major hypotheses have been proposed for the origin of the crustal dichotomy: endogenic (by mantle processes), single impact, or multiple impact. Both impact-related hypotheses involve processes that could have occurred before the end of the primordial bombardment, implying that the crustal dichotomy has its origins early in the history of Mars.

[rogerg]

is Mars Hollow?  

[El_Mayonnaise]

I always keep washing my briefs, I'd hate to get run over by a bus and be found to be wearing dirty underpants  

Cat face! He's got a big cat face!


etc  

[davejd]

I've been stuck in the shower and now i'm not sure if this is all a dream