Large debris objects are typically defined as objects larger than 10 centimetres in size.

Large debris objects are typically defined as objects larger than 10 cm in size.

So this is a plate of nachos.

Eggs or cornflakes?

We sort the plastic fragments into different size classes, from five millimeters to one third of a millimeter.

It could be shown that within the next 100 years collision fragments will dominate the population gt 1 cm.

The cornflake hadn't been invented.

The cornflake hadn't been invented.

The difference between our nachos and the other guy's nachos, is that this is actually a dessert.

She's probably it's a shame you can't see it in the photograph, but she's 12 feet long.

It is hoped that space debris of 2 cm size will be detected in 1000 km range.

The brain is removed from the skull, and then it's sliced into one centimeter slices.

He asked him if he wanted organic Toasted O's or the sugarcoated flakes you know, the one with the big striped cartoon character on the front.

And you can almost trick yourself into thinking you're eating Doritos.

I mean, this was 16 millimeter safety film.

Fried eggs with grated cheese, and lots of cornflakes.

In addition to the sources of space debris that are considered in the modelling of the current debris population, it is necessary to take into account collisions among larger objects ( gt 10 cm).

The cops showed Gaston Noémie's photo.

Within the next 100 years the population gt 1 cm will grow by a factor of 3 to 4, even if the above mentioned mitigation measures will be performed consequently.

This picture is taken at 16 kilometers.

Mr. DeMille is shooting. You got an appointment?

Here's how the great Persian poet Rumi put it Out beyond ideas of wrong doing and right doing, there is a field.

It is stationed at 80 degrees east longitude and measures the submillimetre sized meteoroid and space debris population.

Radar has been the most effective means of observing LEO (low Earth orbit) debris of quot threatening size, quot which is debris pieces larger than about 1 cm.

This leads to a reduced number of initial objects gt 1 cm compared to the previously used population.

Photo 6 Two Mig 23s at Lomé Airport

The north coast of California has rainforests temperate rainforests where it can rain more than 100 inches a year.

Figure IX illustrates the total population of debris particles larger than 1 cm in LEO for a number of scenarios.

Look at that central building right in the middle of the picture that's the 130 foot diameter library, that is exactly the size of the base of the spaceship.

So, this is an image of Diana looking at Camilla kissing her husband, and this was a sequence of images.

and, Do we like the nachos? and, Who is going to win?

And you can almost trick yourself into thinking you're eating Doritos.

Photo 5 Mi 8T bodies being refurbished in Lomé

And the film was shot on 72 millimeter, government issue film.

The picture that emerges from these measurements is that the debris population exceeds the natural meteoroid population for all sizes larger than about 0.01 centimetre in diameter.

The FGAN TIRA system was employed to measure a number of 30 debris objects (sizes larger than 50 cm) selected by NASA, of six small metal spheres of the NASA experiment ODERACS I (orbital debris calibration spheres, diameter of 5 cm, 10 cm, and 15 cm), as well as of three small metal spheres (diameter of 5 cm, 10 cm, 15 cm) and dipoles (two wires of 13.1 cm length and 0.1 cm diameter) of the ODERACS II experiment.

In large tracts of territory there is no system at all.

And the 16mm black and white film gave a different feel to it.

The digital mammogram was read as normal and shows lots of dense tissue, but the MBI shows an area of intense uptake, which correlated with a two centimeter tumor.

These methods and techniques need further improvement and refinement to cope with mid size space debris (size 1 50 cm).

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White board, large