November 15, 2017 Zimmerman/Pratt podcast
My hour-long appearance on Robert Pratt’s Pratt on Texas radio show is now available here.
We had a long discussion about the lack of thoughtful skepticism in today’s intellectual society.
My hour-long appearance on Robert Pratt’s Pratt on Texas radio show is now available here.
We had a long discussion about the lack of thoughtful skepticism in today’s intellectual society.
ARCA has issued a statement following the arrest last week of Dumitru Popescu for embezzlement and fraud.
ARCA Space Corporation will continue the development of its aerospace technology as scheduled. The company has full confidence in CEO Dumitru Popescu and expects him to lead the efforts. Mr. Popescu was charged in New Mexico state courts with alleged embezzlement and securities issues. However, Mr. Popescu maintains his innocence and expects to prevail in court proceedings.
Meanwhile the work of the company will proceed with a goal of presenting a successful aerospike rocket engine.
Capitalism in space: Smallsat rocket company Vector has made a deal with Harris Corporation to use its launch facilities at Vandenberg in California for future launches.
Vector now has arrangements to launch its rockets from Kennedy, from Wallops Island, from Alaska, from the new spaceport in Georgia, and now from Vandenberg. With the rocket designed small enough for easy transportation by truck around the country, this will give them the ability to reach a large variety of orbits while also maintaining a fast launch rate.
The National Science Foundation has found at least one backer to pick up the majority of the cost for running the Arecibo Observatory in Puerto Rico, thus keeping it operational.
For about a decade, the National Science Foundation, which owns the observatory and supplies about two-thirds of its $12 million budget, had been mulling downsizing or even shuttering the telescope to free up funds for other projects. Instead, the NSF will continue scientific operations at the facility in collaboration with an unnamed partner organization, according to a Record of Decision signed this week.
Arecibo sustained $4 million to $8 million in damage during the hurricane, according James Ulvestad, acting assistant director for the agency’s mathematical and physical sciences directorate. Some scientists worried that would weaken the case for keeping the observatory operational.
But Ulvestad said the agency’s Record of Decision reflects that it has received viable partnership proposals from one or more collaborators — though he would not provide details about those proposals. This announcement allows the NSF to move forward with negotiations on a new management contract.
Under the new plan, the agency will reduce its annual contribution to the observatory from about $8.2 million to $2 million over the next five years. It is also committed to funding any repairs required to restore Arecibo to its pre-hurricane condition, Ulvestad said.
Capitalism in space: Virgin Orbit’s LauncherOne has won a contract to launch a Defense Department payload.
The details are vague, but the deal appears real. The article also suggests that Virgin Orbit is on schedule to complete its first launch next year.
Its carrier aircraft, a Boeing 747 that was formerly a passenger airliner for Virgin Atlantic, is currently in flight tests after undergoing modifications to accommodate the launch vehicle. A pathfinder version the rocket, meanwhile, has been shipped from the company’s factory in Long Beach, California to Mojave for testing, including static fire tests of both stages.
All evidence now suggests that my prediction one year ago that this Virgin company will make its first operational flight before Virgin Galactic’s SpaceShipTwo, despite being in development only six years, compared to the fourteen years SpaceShipTwo has been under development.
Capitalism in space: Rocket Lab’s second test Electron rocket has arrived at the company’s New Zealand launch facility in preparation for the rocket’s second flight.
They hope after several weeks of check-out they will be able to announce a launch date. The launch, though intended entirely as a test, will still carry three commercial cubesats, which Rocket Lab hopes to place in orbit.
For the Google Lunar X-Prize contestant Moon Express this launch is critical. They must launch by the end of March to win the prize, and are dependent on Electron as their rocket.
The expected Falcon 9 launch this past week of the mysterious Zuma government payload, built by Northrop Grumman but linked to no government agency, has been postponed indefinitely because of a fairing issue identified during testing for a different customer.
This delay also suggests that this may be an issue that will delay more than one launch, which could effect SpaceX’s effort to achieve 20 launches in 2017.
Capitalim in space: The next to last ULA launch of a Delta 2 rocket successfully launched a $1.6 billion NOAA weather satellite on Saturday.
Embedded below the fold in two parts.
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An evening pause: Performed live in 2015.
Hat tip Edward Thelen.
Because I am off on a caving project this weekend in the mountains where there is no internet service, I will not be able to approve comments or post anything until I return on Sunday.
The next few days should be most interesting, as there are SpaceX and ULA launches scheduled. The SpaceX launch tonight will place a secret government satellite in orbit while trying to land its first stage. The ULA launch on Saturday will be the last launch for its Delta 2 rocket, which the company is retiring because it costs too much to operate.
An evening pause: Hat tip to Edward Thelen for reminding me that I should post another Bowie song. This was recorded live in 1999.
Summary: Curiosity does drill tests, crosses Vera Rubin Ridge. Opportunity finds evidence of either ice or wind scouring on rocks in Perseverance Valley.
For the overall context of Curiosity’s travels, see Pinpointing Curiosity’s location in Gale Crater.
Since my last update on September 6, Curiosity has continued its travels up and across Vera Rubin Ridge, a geological bedding plain dubbed the Hematite Unit. The panorama above, created by reader Phil Veerkamp, shows the view looking up the ridge slope. If you click on it you can see the full resolution image, with lots of interesting geological details.
The panorama below, also created by Veerkamp, shows the view on Sol 1866, two weeks later, as the slope begins to flatten out and the distant foothills of Mount Sharp become visible. (If you click on the image you can see a very slightly reduced version of the full resolution panorama.) This image also shows the next change in geology. From orbit the Hematite Unit darkens suddenly at its higher altitudes, and Curiosity at this point was approaching that transition. The rover is now, on Sol 1876, sitting on that boundary, where they will spend a few days making observations before moving on.
The image on the right shows Curiosity’s approximate position, about halfway across the Hematite Unit and with the rover’s approximate future route indicated, as shown in this October 3, 2016 press release.
In the two months since my last rover update the Curiosity engineering team has spent a lot of time imaging and studying the Hematite Unit. They have also spent a considerable amount of time doing new tests on the rover’s drill in an effort to get around its stuck feed mechanism in order to drill again. Only yesterday they took another series of close-up images of the drill in this continuing effort.
As indicated by the October 3 2016 press release, the rover still has a good way to go before it begins entering the distant canyons and large foothills. While they should leave the Hematite Unit and enter the Clay Unit beyond in only a few more months, I expect it will be at least a year before they pass through the Clay Unit and reach the much more spectacular Sulfate Unit, where the rover will explore at least one deep canyon as well as a recurring dark feature on a slope that scientists think might be a water seep.
For the context of Opportunity’s recent travels along the rim of Endeavour Crater, see my May 15, 2017 rover update.
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Astronomers have announced another black hole merger detected by the LIGO gravitational wave observatory.
Dubbed GW170608, the latest discovery was produced by the merger of two relatively light black holes, 7 and 12 times the mass of the sun, at a distance of about a billion light-years from Earth. The merger left behind a final black hole 18 times the mass of the sun, meaning that energy equivalent to about 1 solar mass was emitted as gravitational waves during the collision.
This event, detected by the two NSF-supported LIGO detectors at 02:01:16 UTC on June 8, 2017 (or 10:01:16 pm on June 7 in US Eastern Daylight time), was actually the second binary black hole merger observed during LIGO’s second observation run since being upgraded in a program called Advanced LIGO. But its announcement was delayed due to the time required to understand two other discoveries: a LIGO-Virgo three-detector observation of gravitational waves from another binary black hole merger (GW170814) on August 14, and the first-ever detection of a binary neutron star merger (GW170817) in light and gravitational waves on August 17.
Archaeologists have found petroglyphs in Saudi Arabia that could be the earliest depiction of dogs being held by leashes.
Carved into a sandstone cliff on the edge of a bygone river in the Arabian Desert, a hunter draws his bow for the kill. He is accompanied by 13 dogs, each with its own coat markings; two animals have lines running from their necks to the man’s waist.
The engravings likely date back more than 8000 years, making them the earliest depictions of dogs, a new study reveals. And those lines are probably leashes, suggesting that humans mastered the art of training and controlling dogs thousands of years earlier than previously thought.
The dating however remains uncertain. The carvings could be much younger.
Using data collected during New Horizons’ fly-by, scientists have found that the planet’s atmosphere is 54º F colder than predicted, and from this they theorize that the presence of haze in that atmosphere is what cools it.
Pluto’s atmosphere is made mostly of nitrogen, with smaller amounts of compounds such as methane. High in the atmosphere — between 500 and 1,000 kilometres above the surface — sunlight triggers chemical reactions that transform some of these gases into solid hydrocarbon particles.
The particles then drift downward and, at around 350 kilometres above Pluto’s surface, clump with others to form long chemical chains. By the time they reach 200 kilometres’ altitude, the particles have transformed into thick layers of haze, which the New Horizons spacecraft saw dramatically blanketing Pluto.
Zhang and his colleagues compared the heating and cooling effects of the atmosphere’s gas molecules to those of its haze particles. Earlier studies have suggested that the presence of gas molecules, such as hydrogen cyanide, could help explain why Pluto’s atmosphere is so cold. But Zhang’s team found that including haze was the only way to get their model to match the temperatures that New Horizons measured as it flew by the dwarf planet.
This theory remains unproven. Moreover, there are other explanations proposed for the cold atmosphere by other scientists. It will take new instruments and future probes to resolve the question.
The post has been corrected. My math in calculating the conversion from Celsius to Fahrenheit was initially faulty. Thanks to reader Kirk for spotting the error.
Link here. He finds much of what he reads, especially involving Virgin Galactic, to be seriously wanting.
Expect a more detailed review in the coming days, but essentially Branson’s dishonest hyperbole shines through.
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Astronomers who have been observing the interstellar object that zipped past the Sun last month have concluded that it mostly resembles asteroids seen in our own solar system.
From its changing brightness, the team inferred that U1 is highly elongated with rough dimensions 30m x 30m x 180m. About twice the height of the Statue of Liberty, the 6:1 aspect ratio of U1 is “similar to the proportions of a fire extinguisher — although U1 is not as red as that,” says David Jewitt (UCLA), the first author of the study.
“With such an elongated shape, U1 probably needs a little cohesive strength to hold it together. But that’s not really unusual,” remarked study coauthor Jayadev Rajagopal (National Optical Astronomy Observatory). Commenting on its size, rotation, and color, Rajagopal mused that, “the most remarkable thing about U1 is that, except for its shape, how familiar and physically unremarkable it is.”
I wonder if they are still tracking it.
An evening pause: I haven’t posted one of these in awhile, and this one is a doozy, including three new US domino records: largest domino field, largest domino structure, and largest overall domino project in America. It took 19 builders from 5 countries 7 days (over 1,200 combined hours) to build it.
As I have noted before, I welcome suggestions for evening pauses. If you have suggested before, please suggest again! And if you have never done so but have something you want to suggest, comment here (without mentioning the suggestion itself) and I will provide you info on how to submit your suggestion.