Video: Space elevator humor

Ted Semon of the The Space Elevator Blog has collected links to all 39 episodes of a series of funny film shorts about four guys on a lift to space : Elevator To Space -The Space Elevator Blog

Several years ago, 4 comics (Alex Koll, Sean Keane, Louis Katz & Chris Garcia) got together to create several short, funny, space-elevator vignettes entitled Elevator To Space.  The premise was four guys in a (building) elevator, riding it up to space.  They created 39 of these videos and they range from mildly humorous to laugh-out-loud funny.

Here are a couple of examples starting with an illustration of how to deal with elevator music on a space elevator:

And the drawbacks of a Mexican style birthday party in a space elevator:

Two families of comets detected around another star

An announcement from the European Southern Observatory (ESO):

Two Families of Comets Found Around Nearby Star
Biggest census ever of exocomets around Beta Pictoris

The HARPS instrument at ESO’s La Silla Observatory in Chile has been used to make the most complete census of comets around another star ever created. A French team of astronomers has studied nearly 500 individual comets orbiting the star Beta Pictoris and has discovered that they belong to two distinct families of exocomets: old exocomets that have made multiple passages near the star, and younger exocomets that probably came from the recent breakup of one or more larger objects. The new results will appear in the journal Nature on 23 October 2014.

Beta Pictoris is a young star located about 63 light-years from the Sun. It is only about 20 million years old and is surrounded by a huge disc of material — a very active young planetary system where gas and dust are produced by the evaporation of comets and the collisions of asteroids.

Flavien Kiefer (IAP/CNRS/UPMC), lead author of the new study sets the scene: “Beta Pictoris is a very exciting target! The detailed observations of its exocomets give us clues to help understand what processes occur in this kind of young planetary system.”

For almost 30 years astronomers have seen subtle changes in the light from Beta Pictoris that were thought to be caused by the passage of comets in front of the star itself. Comets are small bodies of a few kilometres in size, but they are rich in ices, which evaporate when they approach their star, producing gigantic tails of gas and dust that can absorb some of the light passing through them. The dim light from the exocomets is swamped by the light of the brilliant star so they cannot be imaged directly from Earth.

To study the Beta Pictoris exocomets, the team analysed more than 1000 observations obtained between 2003 and 2011 with the HARPS instrument on the ESO 3.6-metre telescope at the La Silla Observatory in Chile.

The researchers selected a sample of 493 different exocomets. Some exocomets were observed several times and for a few hours. Careful analysis provided measurements of the speed and the size of the gas clouds. Some of the orbital properties of each of these exocomets, such as the shape and the orientation of the orbit and the distance to the star, could also be deduced.

This analysis of several hundreds of exocomets in a single exo-planetary system is unique. It revealed the presence of two distinct families of exocomets: one family of old exocomets whose orbits are controlled by a massive planet [1], and another family, probably arising from the recent breakdown of one or a few bigger objects. Different families of comets also exist in the Solar System.

The exocomets of the first family have a variety of orbits and show a rather weak activity with low production rates of gas and dust. This suggests that these comets have exhausted their supplies of ices during their multiple passages close to Beta Pictoris [2].

The exocomets of the second family are much more active and are also on nearly identical orbits [3]. This suggests that the members of the second family all arise from the same origin: probably the breakdown of a larger object whose fragments are on an orbit grazing the star Beta Pictoris.

Flavien Kiefer concludes: “For the first time a statistical study has determined the physics and orbits for a large number of exocomets. This work provides a remarkable look at the mechanisms that were at work in the Solar System just after its formation 4.5 billion years ago.”

Beta Pictoris as Seen in Infrared Light

This composite image represents the close environment of Beta Pictoris as seen in near infrared light. This very faint environment is revealed after a very careful subtraction of the much brighter stellar halo. The outer part of the image shows the reflected light on the dust disc, as observed in 1996 with the ADONIS instrument on ESO’s 3.6 m telescope; the inner part is the innermost part of the system, as seen at 3.6 microns with NACO on the Very Large Telescope. The newly detected source is more than 1000 times fainter than Beta Pictoris, aligned with the disc, at a projected distance of 8 times the Earth-Sun distance. This corresponds to 0.44 arcsecond on the sky, or the angle sustained by a one Euro coin seen at a distance of about 10 kilometres. Because the planet is still very young, it is still very hot, with a temperature around 1200 degrees Celsius. Both parts of the image were obtained on ESO telescopes equipped with adaptive optics.

Credit: ESO/A.-M. Lagrange et al

“Rocket Girl” by George D. Morgan – interview audio and lecture video

On two recent episodes of his Mars Pirate Radio podcast, Doug Turnball interviewed George D. Morgan, author of Rocket Girl: The Story of Mary Sherman Morgan, America’s First Female Rocket Scientist.

Mary Morgan was George’s mother. He originally told her story in a play.

There is a video of George Morgan giving a talk about his mother and about the book from the Sept. 2013 episode of the C-SPAN2 BookTV program: Book Discussion Rocket Girl | Video | C-SPAN.org.

This is from the book description:

An Unsung Heroine of the Space Age – Her Story Finally Told.

This is the extraordinary true story of America’s first female rocket scientist. Told by her son, it describes Mary Sherman Morgan’s crucial contribution to launching America’s first satellite and the author’s labyrinthine journey to uncover his mother’s lost legacy–one buried deep under a lifetime of secrets political, technological, and personal. 

In 1938, a young German rocket enthusiast named Wernher von Braun had dreams of building a rocket that could fly him to the moon. In Ray, North Dakota, a young farm girl named Mary Sherman was attending high school. In an age when girls rarely dreamed of a career in science, Mary wanted to be a chemist. A decade later the dreams of these two disparate individuals would coalesce in ways neither could have imagined. 

World War II and the Cold War space race with the Russians changed the fates of both von Braun and Mary Sherman Morgan. When von Braun and other top engineers could not find a solution to the repeated failures that plagued the nascent US rocket program, North American Aviation, where Sherman Morgan then worked, was given the challenge. Recognizing her talent for chemistry, company management turned the assignment over to young Mary.

In the end, America succeeded in launching rockets into space, but only because of the joint efforts of the brilliant farm girl from North Dakota and the famous German scientist. While von Braun went on to become a high-profile figure in NASA’s manned space flight, Mary Sherman Morgan and her contributions fell into obscurity–until now.