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Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the...

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Collecting and Mapping Planetary Data
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Page 1: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Collecting and Mapping Planetary Data

Page 2: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Direct measurements (in situ)

• Collecting data directly at the site of scientific interest

• Ground stations on Earth

• Landers and atmospheric probes for other planets

Page 3: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Direct measurements (in situ)

Ground Weather Station

Mars Exploration

Rover

Mars Phoenix Lander

Page 4: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Remote Sensing• Gathering information about an object without

coming into direct contact with the object.

Telescopes gather light from distant planets, stars, and galaxies.

Satellites orbiting the Earth collect information about the weather.

Page 5: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Most scientific remote sensing,particularly from satellites, involves

light…

but not necessarily light as you might typically imagine!

Page 6: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

The Electromagnetic Spectrum

• All light has a particular energy, and each energy reveals different information

• Humans are only able to see a small range of these energies, known as the visible spectrum

• Other types of light include gamma rays, x-rays, ultraviolet light, infrared light, and radio waves.

Page 7: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Let’s take a look at some of these different types of light, and

what we can do with them.

Page 8: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Radio Wave Light• Radio waves are the

lowest energy in the spectrum.

• Radio waves are used to transmit radio and television signals and to map the surfaces of planets that are obscured at other wavelengths.

Saturn

Page 9: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Infrared Light• One use of infrared

light is thermal imaging.

• Objects at common Earth temperatures release infrared light that can be used to determine surface temperature.Saturn

Page 10: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Visible Light

• Visible light is the portion of the electromagnetic spectrum that we can detect with our eyes.

• Red light is lower energy than violet light.

• All the colors of the rainbow combine to make white light.

Saturn

Page 11: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Ultraviolet Light

• Some insects, including bees, can see UV light.

• Astronomers can use ultraviolet light to study energetic objects in the universe.

Saturn

Page 12: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

X-Ray Light• X-rays pass through

some objects better than others.

• Medical X-ray images are actually shadows of objects that x-rays could not pass through.

Saturn

Page 13: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Gamma Ray Light• The highest energy in the

electromagnetic spectrum.• Generated by some

radioactive elements and events resulting from nuclear processes.

• Gamma ray light can be used to map elemental composition of planets.

Page 14: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

GRS and THEMIS Remotely Sense Mars

Page 15: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

How are gamma rays and neutrons produced by cosmic rays?

Page 16: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Gamma Ray Animation

Play Gamma Ray Animation

Page 17: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Potassium Map of Mars

Page 18: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Potassium Map of United States

Page 19: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Why Do We Care?

• Although each of these types of light are found in the electromagnetic spectrum, they are created in different ways and give us different types of information.

Page 20: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Remote Sensing• Orbiting satellites can

detect light of various energies.

• Shown here are a visible image of Lake Tahoe and a surface temperature map made with infrared data

• We can represent remote sensing data using false color images.

Page 21: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Mapping Activity

Page 22: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Surface Air Temperature Data

Page 23: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Calculated Soil Moisture DataJuly (1971-2000)

Page 24: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Martian Map of WaterTest for Understanding

Page 25: Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.

Describe the distribution of water on Mars


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