Of course not, but why?
Of course not, but why?
Spitzer, Swift and AstroLAB are now involved in observing this very strange star and now maybe we are getting some answers:
Goddard/NASA – This illustration depicts a hypothetical uneven ring of dust orbiting KIC 8462852, also known as Boyajian’s Star or Tabby’s Star. Astronomers have found the dimming of the star over long periods appears to be weaker at longer infrared wavelengths of light and stronger at shorter ultraviolet wavelengths. Such reddening is characteristic of dust particles and inconsistent with more fanciful “alien megastructure” concepts, which would evenly dim all wavelengths of light.
By studying observations from NASA’s Spitzer and Swift telescopes, as well as the Belgian AstroLAB IRIS observatory, the researchers have been able to better constrain the size of the dust particles. This places them within the range found in dust disks orbiting stars, and larger than the particles typically found in interstellar dust.
The system is portrayed with a couple of comets, consistent with previous studies that have found evidence for cometary activity within the system.
Wait. . . hold on, alien megastuctures?
Well sort of, here watch this TED Talk by none other than astronomer Tabetha Boyajian:
I am trying to figure out how they keep the thermocouple wires to keep from burning off.
NASA – NASA heat shield material that could one day be used on an inflatable aeroshell during atmospheric entry on Mars recently underwent testing at Boeing’s Large Core Arc Tunnel in St. Louis, Missouri.
The inflatable aeroshell, using high temperature advanced flexible material systems, will enable atmospheric entry to planetary bodies and the landing of heavy payloads. The Hypersonic Inflatable Aerodynamic Decelerator (HIAD) project is focused on development of the inflatable aeroshell technology and manufacturing capability at large scale, to support an orbital atmospheric entry flight experiment at Earth and Mars. HIAD overcomes size and weight limitations of current rigid systems by utilizing inflatable soft-goods materials that can be packed into a small volume and deployed to form a large aeroshell before atmospheric entry.
Critical to the development of the technology is development of flexible material systems whose performance must be verified through arc jet testing. During early August testing, small cutouts of the Flexible Thermal Protection System (F-TPS), about 2.5 inches (6.4 cm) in diameter and anywhere from a half-inch (1.3 cm) to 1 inch (2.5 cm) thick, were placed in a supersonic wind tunnel and blasted with jets of superheated plasma gas. The plasma gas hit the cutouts at speeds of Mach 4 or more, and heated the surfaces to temperatures up to approximately 2,700 F. Thermocouples embedded in the samples measured the material’s response to the superheated conditions.
Researchers calibrated tunnel pressure and temperature to be similar to the range of conditions HIADs would face during atmospheric entry on Earth and Mars. The data from these tests will be used to validate mathematical models used for design.
The test team included researchers Steven Tobin, Matt Wells and Andrew Brune of NASA’s Langley Research Center in Hampton, Virginia; and Grant Rossman, a Ph.D. candidate at the Georgia Institute of Technology in Atlanta.
HIAD technology is being developed by researchers at Langley through NASA’s Game Changing Development program, which is part of the agency’s Space Technology Mission Directorate. The program advances space technologies that may lead to entirely new approaches to space missions.
Image: Boeing / NASA
Pretty amazing, catching a solar flare on an iPhone! Not my phone to be sure and I’ve tried. Leave it to ESA, actually they got a lucky break in a way. I want to see the filter they used too!
ESA — A group of astronomers at ESA’s ESTEC were testing some solar observing equipment on 6 September and serendipitously captured a solar flare, which turned out to be one of the most powerful observed in the last decade.
The image shown here was taken with an iPhone through a special interference H-alpha filter (centred at the wavelength of hydrogen emission) mounted to a small dedicated solar telescope at 13:09:26 GMT. An X9.3 flare was observed to launch from the Sun by space telescopes at 12:02 GMT, meaning that this image was taken as the flare was in the gradual decay phase.
The flare is seen as the white cloudy feature with multiple ribbons towards the bottom right of the image. It appears as a lighter feature against the solar background average because of post-flare energy release visible in hydrogen emission from interconnected magnetic loops. North is up.
Wow! Launched on 05 September 1977 Voyager 1 is still flying after 40 years! Congratulations to the Voyager program and NASA!
The image above is the Voyager 40th Anniversary disco poster. Image credit: NASA/JPL-Caltech and you can get your own by clicking here.
If by chance you are near Washington DC and can get to the Smithsonian National Air and Space Museum you can attend the live public event commemorating the event. Most of us will of course not make the journey but no matter we can watch the event live on NASA TV.
Here’s the details from NASA including a link to the live feed:
NASA and the Smithsonian’s National Air and Space Museum will celebrate 40 years of the Voyager 1 & 2 spacecraft — humanity’s farthest and longest-lived mission — with a public event at 12:30 p.m. EDT, Tuesday, Sept. 5.
The observance will take place at the National Air and Space Museum located at Independence Avenue at 6th street SW in Washington. The event will be broadcast live on NASA Television and streamed on the agency’s website.
Activities will include panel discussions about the Voyagers’ creation and mission history, their unprecedented science findings and imagery, impact on Earth’s culture and how the spacecraft inspired countless scientists, engineers and the next generation of explorers. The event also will include a galactic message transmitted toward the Voyager 1 spacecraft by a celebrity guest.
The Voyagers’ original mission was to explore Jupiter and Saturn. Although the twin spacecraft are now far beyond the planets in the solar system, NASA continues to communicate with them daily as they explore the frontier where interstellar space begins.
Participants in the Sept. 5 event are:
The eclipse of 2017 is just a few days away and now I am going to be able to see part of it — weather permitting. I’ll be well north of the line of totality but still will get to see a bite out of the sun. I am so pleased, I’ve seen four solar eclipses of varying degrees, two of them were total and they are just fantastic!
If you are located in the US or parts of Canada, I hope you have good weather!
What if you don’t have glasses? Do not look at the directly without proper eye wear! Fortunately those cardboard glasses are easy to get, I think even some of the public libraries will have some (they are for sure where I will be). Still you could be stuck with no glasses, like construction workers for example, well there is still a simple way to see what is going on. I’ve done this myself with success:
If you get to see the eclipse and can view it safely you will be treated to Bailey’s beads and The diamond ring effect. Here is a great look at them from the 2012 Australian Eclipse in a a video posted by William Hetzel:
The mystery of cosmic rays will be explored in a new detector to be launched to the International Space Station.
The detector is called CREAM short for the Cosmic Ray Energetics And Mass mission. The CREAM detectors have flown before on balloons as far back as 2004 and 2016 at altitudes of around 35 km (120,000 feet) so the technology is not new. This time around being at the ISS, the detector will be able to measure the highest energy cosmic rays so far.
Cosmic rays are constantly raining down on Earth mostly from outside our solar system. Most any astrophotographer has seen evidence of cosmic rays at white pixel anomalies in their photographs.
The launch date: 14 August 2017
More information on CREAM and cosmic rays.
I’ve seen a few different views of Larsen C and this image from ESA’s Sentinel-1 spacecraft is one of the best and arguably the most interesting.
ESA — On 12 July 2017, Europe’s Copernicus Sentinel-1 mission returned radar images showing that a lump of ice more than twice the size of Luxembourg had broken off the Antarctic Peninsula. Since then, this large tabular iceberg – known as A68 – has drifted about 5 km from the ice shelf. Images from Sentinel-1 also show that a cluster of more than 11 smaller icebergs has also now formed, the largest of which is over 13 km long. These ‘bergy bits’ have broken off both the giant iceberg and the remaining ice shelf. The image has been compiled using Sentinel-1 acquisitions on 27 July (right) and 30 July (left).
Image contains modified Copernicus Sentinel data (2017), processed by BAS–A. Fleming.