Friday, July 12, 2019

If everyone cares about Mars more, why are we going back to the moon?


If everyone cares about Mars more, why are we going back to the moon? 
Source: DW
Neil Armstrong and Buzz Aldrin's initial Apollo 11 moon landing was more of a political triumph over the Soviet Union than a scientific one – the mission lasted just 3 days, and little actual scientific work was performed.
However, in the following Apollo missions, astronauts collected rocks allowing scientists to better understand the composition of the moon's surface, many of which they preserved for later generations with better technology to study.
With new remote sensing technology, scientists recently discovered the existence of water on the north and south poles of the moon. This discovery, paired with the knowledge acquired from the preserved moon rock, will better guide Artemis venturers on a quest to discover lunar water.
The existence of this water could be fairly groundbreaking if, with further exploration, more is discovered and scientists are able to find ways to extract it. An ample supply of lunar water could help support a space station on the moon - which was previously considered unlikely due to a general understanding that the moon was drier than the Sahara.
At this point, if anyone wants to colonize Mars, they will need to take laborious, energy-heavy trips from Earth lasting up to 8 months one-way. A moon station could help mitigate the lengthy journey, according to planetary geologist Georgiana Kramer. This could save Mars-faring rockets time, energy and money. 
Can we use lunar water?
Because the moon isn't tilted on an axis, like Earth, the poles receive no sunlight at all. Water ice exists in deep craters on these poles, where Artemis plans to land.
NASA planetary geologist Sarah Noble said the source of the water is still unknown, but that it could be the result of comet and meteorite deposition (because the moon has no atmosphere to ward them off); solar winds from the sun, which could bring hydrogen that mixes with oxygen-hosting minerals on the moon's surface; or early lunar volcanism, which could have released water that is still trapped.
Early lunar volcanism also created lava tubes, which are also found on Earth in volcanic areas in Hawaii and Colorado. They are long, cave-like tunnels on the surface of the moon, where lava once flowed and has now cooled.
When the feasibility of life on the moon is discussed in online forums such as Reddit, the idea of placing a space station inside one of the lava tubes is often raised. Both Kramer and Noble confirm this could potentially work, depending on what's discovered during the Artemis mission. The rock, Kramer said, could shield the sun's radiation and feature relatively normalized temperatures.
Noble said in the short term, life in the tubes isn't part of NASA's plan, but in the long term, they could be investigated by robots.
It will be impossible to know whether these theories are accurate until scientists are able to sample the water, however, which is why Artemis plans to land on the south pole of the moon, where much of it is concentrated. Up to this point, scientists haven't had any physical interactions with lunar water, Kramer said.
If a good amount of water is discovered, it could be used for rocket fuel and drinking, which could make Mars exploration easier. 
Which place is better for life: Mars or the moon?
All of that said, Mars simply has more resources than the moon, Robert Zubrin, an aerospace engineer, wrote in a treatise published by the National Space Society's magazine "Ad Astra".
"In contrast to the Moon, Mars is rich in carbon, nitrogen, hydrogen and oxygen, all in biologically readily accessible forms such as carbon dioxide gas, nitrogen gas, and water ice and permafrost. Carbon, nitrogen, and hydrogen are only present on the Moon in parts per million quantities, much like gold in seawater," he wrote.
Zubrin is the author of Mars Direct, a research paper-turned-book advocating for Mars exploration, and heads the Mars Society, which also advocates for Mars exploration.
The moon does not receive enough natural sunlight to grow plants of any variety, Zubrin writes, but Mars does, which will allow future colonists to sustain themselves in a way they never could on the moon.
This is all in addition to the moon's lack of an atmosphere, extreme weather changes and barren, radioactive surface.
Zubrin's analysis of Mars illustrates why life on the moon is only considered in the context of the lunar body serving as a stopping-off point on the way to something bigger and better - or, at least, more sustainable for human populations.


Friday, July 5, 2019

Earthquake Magnitude


Earthquake Magnitude
Source: U.S. Geological Survey (USGS) 
Earthquake magnitude, energy release, and shaking intensity are all related measurements of an earthquake that are often confused with one another. Their dependencies and relationships can be complicated, and even one of these concepts alone can be confusing.

Magnitude


The time, location, and magnitude of an earthquake can be determined from the data recorded by seismometer. Seismometers record the vibrations from earthquakes that travel through the Earth. Each seismometer records the shaking of the ground directly beneath it. Sensitive instruments, which greatly magnify these ground motions, can detect strong earthquakes from sources anywhere in the world. Modern systems precisely amplify and record ground motion (typically at periods of between 0.1 and 100 seconds) as a function of time.

Types of Magnitudes

Magnitude is expressed in whole numbers and decimal fractions. For example, a magnitude 5.3 is a moderate earthquake, and a 6.3 is a strong earthquake. Because of the logarithmic basis of the scale, each whole number increase in magnitude represents a tenfold increase in measured amplitude... of what? (Richter only?).
When initially developed, all magnitude scales based on measurements of the recorded waveform amplitudes were thought to be equivalent. But for very large earthquakes, some magnitudes underestimate true earthquake size, and some underestimate the size. Thus, we now use measurements that describe the physical effects of an earthquake rather than measurements based only on the amplitude of a waveform recording. More on that later.


The Richter Scale (ML) is what most people have heard about, but in practice it is not commonly used anymore, except for small earthquakes recorded locally, for which ML and short-period surface wave magnitude (Mblg) are the only magnitudes that can be measured. For all other earthquakes, the moment magnitude (Mw) scale is a more accurate measure of the earthquake size.
Although similar seismographs had existed since the 1890's, it was only in 1935 that Charles F. Richter, a seismologist at the California Institute of Technology, introduced the concept of earthquake magnitude. His original definition held only for California earthquakes occurring within 600 km of a particular type of seismograph (the Woods-Anderson torsion instrument). His basic idea was quite simple: by knowing the distance from a seismograph to an earthquake and observing the maximum signal amplitude recorded on the seismograph, an empirical quantitative ranking of the earthquake's inherent size or strength could be made. Most California earthquakes occur within the top 16 km of the crust; to a first approximation, corrections for variations in earthquake focal depth were, therefore, unnecessary.
The Richter magnitude of an earthquake is determined from the logarithm of the amplitude of waves recorded by seismographs. Adjustments are included for the variation in the distance between the various seismographs and the epicenter of the earthquakes.
Moment Magnitude (MW) is based on physical properties of the earthquake derived from an analysis of all the waveforms recorded from the shaking. First the seismic moment is computed, and then it is converted to a magnitude designed to be roughly equal to the Richter Scale in the magnitude range where they overlap.
Moment (MO) = rigidity x area x slip
where rigidity is the strength of the rock along the fault, area is the area of the fault that slipped, and slip is the distance the fault moved. Thus, stronger rock material, or a larger area, or more movement in an earthquake will all contribute to produce a larger magnitude.
Then,
Moment Magnitude (MW) = 2/3 log10(MO) - 10.7

Energy Release


Earthquake magnitudes and energy release, and comparison with other natural and man-made events. (Gavin Hayes)
Another way to measure the size of an earthquake is to compute how much energy it released. The amount of energy radiated by an earthquake is a measure of the potential for damage to man-made structures. An earthquake releases energy at many frequencies, and in order to compute an accurate value, you have to include all frequencies of shaking for the entire event.
While each whole number increase in magnitude represents a tenfold increase in the measured amplitude, it represents a 32 times more energy release.
The energy can be converted into yet another magnitude type called the Energy Magnitude (Me). However, since the Energy Magnitude and Moment Magnitude measure two different properties of the earthquake, their values are not the same.
The energy release can also be roughly estimated by converting the moment magnitude to energy using the equation log E = 5.24 + 1.44M, where M is the magnitude.

Intensity

Whereas the magnitude of an earthquake is one value that describes the size, there are many intensity values for each earthquake that are distributed across the geographic area around the earthquake epicenter. The intensity is the measure of shaking at each location, and this varies from place to place, depending mostly on the distance from the fault rupture area. However, there are many more aspects of the earthquake and the ground it shakes that affect the intensity at each location, such as what direction the earthquake ruptured, and what type of surface geology is directly beneath you. Intensities are expressed in Roman numerals, for example, VI, X, etc.
Traditionally the intensity is a subjective measure derived from human observations and reports of felt shaking and damage. The data used to be gathered from postal questionnaires, but with the advent of the internet, it's now collected using a web-based form. However, instrumental data at each station location can be used to calculate an estimated intensity.