Borah Peak Fault Scarp in Idaho formed during 1983 Quake

The thin tan line in this photo is the Lost River Fault Scarp, which runs for over 20 miles along the base of the Lost River Range in central Idaho. The scarp formed as result of a 6.9 M earthquake that occurred at 8:06 am on October 28, 1983. The quake was named the “Borah Peak Earthquake” because it happened near Borah Peak (12,662 ft.), the highest mountain in Idaho - the one on the left in this photograph. The photo was taken along the road to the Birch Springs Trailhead where hundreds of hikers come every year to begin their ascent of Borah (known locally as Mt. Borah).

The Lost River Range is a fault-block mountain range on the northeastern edge of the Basin and Range Province. Like Basin and Range Mountains in other states such as Utah and Nevada, these mountains formed one earthquake at a time over millions of years. During the 1983 quake the valley side of the fault dropped 9 feet and the block that includes the Lost River Range rose 6 inches, leaving the offset (scarp) shown in the photos.

The epicenter was located along the fault somewhere between the small towns of Mckay and Challis. Although it was the most energetic earthquake in the lower 48 since the 1959 Hebgen Lake Earthquake in southwestern Montana, there were only two deaths. Two children (ages 6 and 7) were killed in Challis when a brick wall collapsed on them as they walked to school. Shaking was felt in eight states and two Canadian provinces, lasting from 30-60 seconds.

Below: This photo, taken by Bruce Railsback of the University of Georgia, shows a person standing below the Lost River Fault Scarp (near bottom, center of photo). Bruce took the photo in in 1987, four years after the earthquake happened.

Links . . .

Newspaper coverage by the Idaho Statesman

Basin and Range Province (Wikipedia)

Climbing Mt. Borah (aka Borah Peak)

Fault-Block Mountains (Wikipedia)

Animation of the Night Sky at Your Location

CLICK HERE to go to Timeanddate.com, set the site to your location (or a nearby city), scroll down to the "Night Sky Map", select a planet to watch, and then click on the play arrow (or FFWD arrow, or scroll bar). You can pause and scroll over stars or other planets to see their names. Pretty dang cool if you ask me! The site provides plenty of other interactive astronomy animations to fiddle around with as well.

Below: This screen shot is an example of what you will see - except it will be in motion. NOTE: The site resets at noon every day, so the best time to check is afternoon.

Draw the orbits of the planets on your city.

This is a really cool way to help students understand the size of the solar system. Go to this website, and center the map on your city. This can be done entering your latitude and longitude, or you can expand the map* to full screen and then manipulate it so that your city is at the center. Then enter "33223 mm" for the diameter of the Sun - This is how big the Sun would be if the Earth were the size of a standard globe (12 inches in diameter). Finally, select "calculate" and "show orbits".

*If you expand the map to "full screen" you will need to get out of "full screen" to enter the diameter of the Sun.

Below: To see where the planets are right now, go to this website.

Losing Ground - a documentary about urban sprawl

Maybe we (Earth Science teachers) should spend more time teaching students about soil (the forgotten natural resouce) and help students understand this issue. We lose 175 acres of land to urban sprawl every hour! The documentary will premiere on May 27,2019 and then will be available on the "Angus TV" YouTube Channel after that - Mark your calendar.

Kelvin-Helmholtz Clouds Caused by Wind Shear

The right place, at the right time.
This photo of an amazing Kelvin-Helmholtz cloud was taken on January 26, 2019 by Hannah Martin, one of my freshman Earth Science students at Helena High School. She snapped the photo from the Helena Valley, looking west - Mount Helena can be seen on the left, and the distant horizon marks the Continental Divide. Also known as "fluctus" or "billow" clouds, they were named after Lord Kelvin (1824-1907) and Hermann Von Helmholtz (1821-1894) who identified the type of instability responsible for the unique waves. Such clouds are fairly rare, and may only last for a few minutes.

Like wind across water.
The waves form at the boundary between layers of air that have different densities and wind speeds (wind shear). Air in the layer above the cloud is moving faster than air in the layer containing the cloud. Development of waves on the cloudy layer is similar to what happens when waves form on the ocean as wind blows across the water. In the photo the wavy layer is more dense than the clear air flowing above it - just as water is more dense than air blowing over its surface.

Clouds provide a "visual".
The type of motion that causes the wave pattern is actually not that uncommon in the atmosphere, although we usually don't see it. In order for us to see it, clouds must be present in the lower layer (as they were when the photo was taken). We can't see clear air, but we can see clouds. One of the nice things about clouds is they provide clues about the type of motion currently happening in the atmosphere. Want to know more? - Watch the 4.5-minute video below, which includes a great demo.

Term for students to define: wind shear

1. Article - More about KH Clouds

2. Another good article about KH Clouds

Check out the Lunar Eclipse on Sunday, January 20th.

The eclipse will start at 7:36 pm MST, and will about 5 hours from start to finish. Hopefully it will be clear where you live! To find out more about the timing, etc., here are a couple resources . . .

1. Go to timeanddate.com and enter your location.

2. Read how to watch at theverge.com.

The video below is not specific to the eclipse of January 2019, but it does an nice job of explaining different aspects of lunar eclipses.

Enter your address to see where you would have been millions of years ago.

This is a fantastic interactive visualization that was created (and is maintained) by Ian Webster. Once the site opens, enter your address in the box in the upper left, then select the time (in Earth's history) near the top of the web page. To see more of Ian's work, go to ianww.com.

Thanks to Rick Dees for showing me this!