How will the Moon look on any date in 2018? What will it look like on your birthday? Find out at NASA Dial-a-Moon. Enter any month, day, and universal time (UT) hour to see a high definition image. The composite images of Dial-a-Moon are made from those of the Lunar Reconnaissance Orbiter (LRO) in low altitude orbit around the Moon since 2009. Here is the link for southern hemisphere readers.
You may leave the universal time (UT) at the default 1 value. If you are a curious type, Universal time conversion can be done at this link. Enter UTC in the lower right box if it isn’t already set. You can switch from 12 hr to 24 hr at the bottom of the entry boxes. You may also enter any other local time in the upper left box. Go back to Dial-a-Moon to enter the UT.
The collection of accurate images of the Moon for each hour have been made into a movie lasting about 5 minutes. Try watching full screen. Versions of the movie are available for readers in the northern and the southern hemispheres.
I explain the peculiar wobble and tipping motions at this blog post.
In case you didn’t notice, the predicted end of the world on 19 Nov 2017 did not happen. I don’t expect it to happen any time soon. I don’t normally make bold predictions about anything. There was one exception in 1974 in the Nixon administration. I successfully predicted he would resign. I think I was lucky.
If you are a believer in the end times prophesies, you may scoff at my prediction. That’s ok. I will give 10 reasons why I think I’m right. Mine are based on science. Join me below the glowing solar firestorm of death and destruction for the reasons we can feel the end is NOT near.
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My bags are packed. I am ready to join 2.4 million other passengers as we begin our journey to Mars in May 2018 aboard the INSIGHT spacecraft. The trip will take about 7 months. It is a one-way journey.
Click to read the fine print. My flight miles award will be enormous.
INSIGHT is the acronym for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport. NASA loves acronyms. Previous Mars missions have studied intensively the surface and atmosphere of the planet. This spacecraft is the first designed to study the interior in hopes of finding clues to the formation of the rocky inner planets. The spacecraft will use seismology, heat flow equipment, and very precise tracking to probe the planet below ground.
The opportunity to sign up for the mission ended on November 1. There were over 2.4 million people who did so. In this link are examples which include children from an elementary school, mission and science managers, as well as famous people like William Shatner.
Clinton Prairie Elementary School | Frankfort, Indiana
Our names will be placed on silicon microchips and attached to the spacecraft. I think it is cool that so many names will be planted on another planet. Perhaps future space travelers will find them. Would you be willing to make the actual trip knowing it was one-way?
The sun’s output in the visible spectrum peaks around yellow. Our eyes are most sensitive to that part of the visible spectrum. The sun also radiates in a broad range of other wavelengths invisible to our eyes. Each comes from dynamics taking place on the surface and in the atmosphere of the sun.
I’ve written about NASA’s Solar Dynamics Observatory (SDO) earlier in a previous post. SDO observes and images the sun several times a minute at ten different wavelengths to give a more complete picture of the activity at and near the surface. A description of those wavelengths is available here. I used the images from the SDO site to render this image of the sun at those ten wavelengths. The yellow center represents the sun’s surface. Each ring of color is at a higher altitude and temperature in the atmosphere of the sun.
Original images used from: NASA/GSFC/Solar Dynamics Observatory
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Have you considered doing a DNA test? We both had our DNA tested in 2014 by 23andMe. The 23andMe results were interesting. We have thorough genealogy records for most of our family lines going back many generations. We knew what to expect from our DNA results.
My last name is derived from a variation of Raudenbusch near Stuttgart Germany. They came to Philadelphia in 1732 according to the ship manifest. The name was changed after a generation to avoid confusion with other Raudenbusch families who lived nearby. The French & German part of the chart below from 23andMe confirms that information.
They married into family lines that were British & Irish, my most recent ancestors in the timeline chart. The results also showed distant generations from Africa making up a very small part of my DNA. My records show distant relatives on my mother’s side from South Carolina who owned slaves in the late 1700s. The genetic link from 23andMe isn’t a surprise.
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The Cassini-Huygens mission has delivered an enormous amount of new scientific findings about Saturn, its rings, and the surrounding many moons. Design work on the mission started in the 1980s as a joint effort by NASA, the European Space Agency ESA, and the Italian space agency Agenzia Spaziale Italiana ASI. Launch was on 15 October 1997. It reached Saturn orbit 1 July 2004 after flybys of Venus, Earth, and Jupiter to adjust the orbit speed and direction via gravity assist. My previous posts about many of the findings by Cassini and Huygens are listed here.
On 15 September 2017, the Cassini spacecraft ends the mission by plunging into the atmosphere of Saturn. It will not be left in orbit for fear of collision with a Saturnian moon and possible contamination of the moon. Future missions to the Saturn system need to be free of any potential contaminants from Earth.
Some scientists and mission specialists have worked on Cassini for their entire careers. This video highlights a few of them and how they feel about the legacy of the mission. I congratulate them all for a job well done. I will be watching NASA-TV at 6 am CDT September 15 to see the final moments of the plunge into Saturn. I hope you will be watching, too.
MinutePhysics author Henry Reich on YouTube explains the physics of a phenomenon in a minute if possible. Here he explains what is left behind when stars die. The corpse of the star depends on what mass the star had in the beginning. He took more than a minute, but less than three. I think that is quite good.
My previous post about this topic describes how stars change over time. Fair warning: It will take more than a minute to read. Probably more than three minutes.