500 protesters block access road on Mauna Kea

About 500 protesters this morning blocked the access road on Mauna Kea that construction vehicles were going to use to begin construction of the Thirty Meter Telescope (TMT).

More than 500 protestors blocked Mauna Kea Access Road and chanted at the sun rose this morning, including seven who chained themselves to a cattle guard near the base of the road.

A convoy of state Department of Transportation vehicles carrying traffic control signage passed the intersection but made no effort to turn onto the access road.

More than a dozen elders with the protest movement sat on folding chairs and were joined by two protestors in wheelchairs at the bottom to the road as the crowd chanted and sang.

Police made no effort to disturb the protest. Gov. David Ige announced last week that the access road would be closed at 7 a.m. today to clear the way for heavy equipment for the controversial $1.4 billion Thirty Meter Telescope.

Based on this report it sounds like the protesters have successfully prevented construction from beginning.

Several points: First, these protesters are breaking the law.

Second, these protesters had their day in court, and lost. In a civilized society, you accept such decisions. No civilization can function if some people think they will always get their way, even if the law and the majority rule against them.

Third, at this moment it appears that David Ige, the Democratic governor, is doing exactly what I expected. He is mouthing platitudes about supporting the law and the construction, while allowing the protesters to block it. Unless he takes action in the next day or so to remove the protesters and clear the road, the protests will grow and become unmanageable. At that point Ige will say that construction must be stopped to avoid bloodshed, and to honor the wishes of what must be a large percentage of the population.

That last part however is a lie. Polls have all indicated that the public wants TMT. And the law is on the public’s side here. It is Ige’s job to support both, not a small minority of unruly spoiled agitators.

Being a modern Democrat however, I expect Ige to favor the lawbreakers.

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TMT construction begins July 15

According to a press announcement today from the governor’s office in Hawaii, construction of the Thirty Meter Telescope will finally begin during the week of July 15 following several years of delays due to protests.

The State Department of Transportation announced that Mauna Kea Access Road will be closed and there could be lane and other road closures associated with large equipment movement beginning July 15. In addition, hunting units A, K, and G in the Mauna Kea Forest Reserve area will be temporarily closed to hunting effective July 15. Both measures are being taken to ensure the safety and security of the public and personnel involved in moving equipment for the TMT project up the Mauna Kea Access Road.

Expect more protests. The real question is whether the Democratic governor David Ige can stand up to them, especially because these protesters have been using the kind of identity politics that the Democratic Party relies on. Ige would have to defy that, and I haven’t seen a Democrat do that in decades.

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Astronomers find kilometer-sized asteroid with shortest year

Astronomers have found a kilometer-sized asteroid with a year only 151 days long, the shortest year of any asteroid.

The asteroid has been dubbed 2019 LF6.

In its orbit, the asteroid swings out beyond Venus and, at times, comes closer in than Mercury, which circles the sun every 88 days. 2019 LF6 is one of only 20 known “Atira” asteroids, which are objects whose orbits fall entirely within Earth’s.

Atira asteroids are difficult to find because they are so close to the Sun, which makes observations difficult if not impossible. Expect more such discoveries as the technology to make these observations improves.

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Astronomers map exoplanet atmosphere of super-Earth

Worlds without end: Using both the Hubble and Spitzer space telescopes, astronomers have characterized the atmosphere of an exoplanet with a mass between that of the Earth and Neptune.

Astronomers enlisted the combined multi-wavelength capabilities NASA’s Hubble snd Spitzer space telescopes to do a first-of-a-kind study of GJ 3470 b’s atmosphere. This was accomplished by measuring the absorption of starlight as the planet passed in front of its star (transit) and the loss of reflected light from the planet as it passed behind the star (eclipse). All totaled, the space telescopes observed 12 transits and 20 eclipses. The science of analyzing chemical fingerprints based on light is called “spectroscopy.”

“For the first time we have a spectroscopic signature of such a world,” said Benneke. But he is at a loss for classification: Should it be called a “super-Earth” or “sub-Neptune?” Or perhaps something else?

Fortuitously, the atmosphere of GJ 3470 b turned out to be mostly clear, with only thin hazes, enabling the scientists to probe deep into the atmosphere. “We expected an atmosphere strongly enriched in heavier elements like oxygen and carbon which are forming abundant water vapor and methane gas, similar to what we see on Neptune”, said Benneke. “Instead, we found an atmosphere that is so poor in heavy elements that its composition resembles the hydrogen/helium rich composition of the Sun.”

To me, our knowledge of exoplanets today is beginning to resemble our knowledge of the planets in the solar system c. 1950. The little data we have gives us a vague idea of what’s there, but there are so many gaps and uncertainties that no one should be confident about drawing any firm conclusions.

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New image of Eta Carina from Hubble

Eta Carina
Click for full image.

Using the Hubble Space Telescope, astronomers have taken a new spectacular image of the Luminous Blue Giant star Eta Carina. The image on the right is that photograph, reduced to post here.

Using Hubble’s Wide Field Camera 3 to map the ultraviolet-light glow of magnesium embedded in warm gas (shown in blue), astronomers were surprised to discover the gas in places they had not seen it before.

Scientists have long known that the outer material thrown off in the 1840s eruption has been heated by shock waves after crashing into the doomed star’s previously ejected material. In the new images, the team had expected to find light from magnesium coming from the same complicated array of filaments as seen in the glowing nitrogen (shown in red). Instead, a completely new luminous magnesium structure was found in the space between the dusty bipolar bubbles and the outer shock-heated nitrogen-rich filaments.

Eta Carina had a major eruption in the 1840s, followed by other lesser outbursts, the evidence of which is obvious in this and other earlier Hubble images. In fact, over the past twenty-five years Hubble has actually tracked the expansion of those two lobes of material being flung from the star hidden deep in the material.

Someday in the far future astronomers believe it will die as a supernova, though that is only a hypothesis at this point, based on our presently limited understanding of stellar evolution.

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TESS finds exoplanet smaller than Earth

Worlds without end: TESS has now found an exoplanet somewhere between Mars and the Earth in size, and is part of a solar system with two other Earth-sized planets.

L 98-59b is around 80% Earth’s size and about 10% smaller than the previous record holder discovered by TESS. Its host star, L 98-59, is an M dwarf about one-third the mass of the Sun and lies about 35 light-years away in the southern constellation Volans. While L 98-59b is a record for TESS, even smaller planets have been discovered in data collected by NASA’s Kepler satellite, including Kepler-37b, which is only 20% larger than the Moon.

The two other worlds in the system, L 98-59c and L 98-59d, are respectively around 1.4 and 1.6 times Earth’s size. All three were discovered by TESS using transits, periodic dips in the star’s brightness caused when each planet passes in front of it.

None of these planets is considered in the habitable zone however. Instead, they experience solar energies comparable to Venus.

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Fast radio burst located for the first time

Astronomers have for the first time pinpointed the location of a non-repeating fast radio burst.

In a historic first, an international team of researchers have discovered the source of a non-repeating fast radio burst and traced its origin to a galaxy 4 billion light-years away.

The monumental findings, published in AAAS journal Science on Thursday, detail the discovery and localization of FRB 180924, a powerful, one-off fast radio burst that lasted for just a fraction of a second. Speculation about the cause of the bizarre signals takes in everything from explosive neutron stars to alien spacecraft, and while we’re still not sure what’s causing them, the revelation puts astronomers one step closer to their true nature.

“This is the big breakthrough that the field has been waiting for since astronomers discovered fast radio bursts in 2007,” said Keith Bannister, lead author of the paper and principal research engineer with Australia’s Commonwealth Scientific and Industrial Research Organisation.

Knowing the distance for the burst makes it possible to calculate how powerful it was, which helps theorists come up with an explanation for what might have caused it. Similarly, knowing its location–on the outskirts of a spiral galaxy like the Milky Way–helps them further constrain those theories.

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The Whirlpool Galaxy across many wavelengths

The Whirlpool Galaxy
Click for full image.

Cool image time! The sequence of images above, reduced to post here, were taken in multiple wavelengths by the 2.1 meter Kitt Peak National Observatory in Arizona and the Spitzer Space Telescope in orbit.

The Whirlpool galaxy, also known as Messier 51 and NGC 5194/5195, is actually a pair of galaxies that are tugging and distorting each other through their mutual gravitational attraction. Located approximately 23 million light-years away, it resides in the constellation Canes Venatici.

The leftmost panel shows the Whirlpool in visible light, much as our eye might see it through a powerful telescope. In fact, this image comes from the Kitt Peak National Observatory 2.1-meter (6.8-foot) telescope. The spiraling arms are laced with dark threads of dust that radiate little visible light and obscure stars positioned within or behind them.

The second panel from the left includes two visible-light wavelengths (in blue and green) from Kitt Peak but adds Spitzer’s infrared data in red. This emphasizes how the dark dust veins that block our view in visible light begin to light up at these longer, infrared wavelengths.

Spitzer’s full infrared view can be seen in the right two panels, which cover slightly different ranges of infrared light.

The infrared views of the Whirlpool galaxy also show how dramatically different its two component parts are: The smaller companion galaxy at the top of the image has been stripped nearly clean of dust features that stand out so brilliantly in the lower spiral galaxy. The faint bluish haze seen around the upper galaxy is likely the blended light from stars thrown out of the galaxies as these two objects pull at each other during their close approach.

The Spitzer images above are likely among the last we shall see from that telescope, which has been in orbit since 2003 with a planned mission of only 2.5 years. As its cryogenic coolant became depleted in 2009, it has been functioning in a somewhat limited phase since. NASA will officially end the mission on January 30, 2020, more than thirteen years beyond that initial lifespan.

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Battery screw-up delays Russian X-Ray telescope launch

The Russians this morning postponed today’s launch of the Spectr-RG X-Ray space telescope until July when it was discovered that one of the payload’s batteries had been drained prematurely.

[T]he Moskovsky Komsomolets tabloid reported from Baikonur that the problem had been discovered at least a day earlier, but the entire project team at the launch site was kept in the dark until the launch date, not to interfere with Vladimir Putin’s annual press-conference.

According to the paper, the battery was accidentally activated on the launch pad instead of the planned moment after the separation of the spacecraft from the Block DM-03 upper stage. The error was blamed on the erroneous wiring setup by RKK Energia specialists (Block DM-03 prime contractor) between the upper stage and the spacecraft, which caused a complete drainage of the battery designed to be re-charged from solar panels. After the return of the rocket to the vehicle assembly building, the battery would have to be re-charged and the power-supply system re-wired, Moskovsky Komsomolets said. [emphasis mine]

If this report is true, it appears that the Russian government has done nothing to fix the quality control programs in its aerospace industry, and in fact is helping to contribute to them by playing games with launch procedures for the sake of its own public relations.

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Hawaii fully okays construction of TMT, removes protest structures

The Hawaiian state government today finally gave the go-ahead for the construction of the Thirty Meter Telescope (TMT), sending close to 100 police officers to the mountain to remove four structures built by protesters to block construction.

[Democratic government David] Ige said he believes the state now has sufficient legal basis for construction to go more smoothly than it did following the telescope’s 2014 groundbreaking. After significant protests in 2014 and 2015, the state Supreme Court ruled in 2015 that a 2011 permit from the state Board of Land and Natural Resources was invalid after finding the Land Board violated due process rights of project opponents by voting before the first contested case was held.

However, the Supreme Court approved an amended permit late last year, allowing the project to seek a notice to proceed. The conditions of the amended permit state that the TMT will be the last telescope to be built on Maunakea and that five other telescopes at the summit will be decommissioned and removed.

Despite Ige’s confidence in the process, opponents are preparing for further protests. Kanuha said he intends to “try and stop it the same way we did the first time.”

“This is about more than the mountain, this is about how we treat land and natural resources in Hawaii,” Kanuha said. “If we allow this to happen, we can kiss goodbye all we hold precious in Hawaii. It’s just a matter of time.”

Another protester, Lakea Trask, warned of an inevitable conflict. “The state is declaring war on Hawaiians,” said Trask, who was arrested and charged with trespassing during the 2015 protests. “The state is now using TMT to declare war, an all-out war on Hawaiians.”

First, this is the second time the state has approved this project, which followed the law both the first time and now. Second, the protests that stopped construction in 2014 and 2015 were not “significant” but were led by a very small number of people. Third, those same protesters, as quoted above, probably intend to repeat their actions once construction resumes this summer. If so, expect violence. These people know they will not be seriously punished for breaking the law, and will take advantage of this.

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The make-up and temperature of Uranus’s rings

The rings of Uranus

New radio images taken by the ground-based telescopes by the ALMA and VLT telescopes in Chile have allowed scientists to better determine the make-up and temperature of the rings of Uranus.

The image above is from their paper. From the caption:

Images of the Uranian ring system at 3.1 mm (ALMA Band 3; 97.5 GHz), 2.1 mm (ALMA Band 4; 144 GHz), 1.3 mm (ALMA Band 6; 233 GHz), and 18.7 μm (VLT VISIR; 100 THz)…The planet itself is masked since it is very bright compared to the rings.

From the article above:

The new images taken by the Atacama Large Millimeter/submillimeter Array (ALMA) and the Very Large Telescope (VLT) allowed the team for the first time to measure the temperature of the rings: a cool 77 Kelvin, or 77 degrees above absolute zero — the boiling temperature of liquid nitrogen and equivalent to 320 degrees below zero Fahrenheit.

The observations also confirm that Uranus’s brightest and densest ring, called the epsilon ring, differs from the other known ring systems within our solar system, in particular the spectacularly beautiful rings of Saturn.

“Saturn’s mainly icy rings are broad, bright and have a range of particle sizes, from micron-sized dust in the innermost D ring, to tens of meters in size in the main rings,” said Imke de Pater, a UC Berkeley professor of astronomy. “The small end is missing in the main rings of Uranus; the brightest ring, epsilon, is composed of golf ball-sized and larger rocks.” [emphasis mine]

The mystery is why this ring has no dust, something not seen with any other ring system in the solar system, including the inner rings of Uranus itself..

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Two Earthlike planets possibly found around neaby red dwarf star

The uncertainty of science: Astronomers think they may have detected evidence of two Earth-sized planets orbiting a tiny red dwarf star only twelve light years away.

Ribas and his colleagues are currently searching for planets orbiting 342 small stars, so they aimed the CARMENES instrument, located at Spain’s Calar Alto Observatory, at the mini-star.

CARMENES observed Teegarden’s star over three years, watching for the wiggles and tugs produced by any orbiting planets. In the end, more than 200 measurements suggested that two small worlds are jostling the star, each weighing in at approximately 1.1 times Earth’s mass. The team calculates that one of the planets, called Teegarden’s star b, completed an orbit in a mere 4.9 Earth-days; the other world, Teegarden’s star c, has an orbit of just 11.4 days.

There is great uncertainty in these results, as the article correctly notes. However, if confirmed these planets could be the home of a very ancient civilization, considering that the red dwarf star is already twice as old as our Sun. There also could be no life there at all, as red dwarf stars tend to be very lacking in many of the materials needed for life.

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