Back again. Star gazing again.

August 10th, 2022

Yea, yea, yea, I know. I’ve been slack but I had to take a hiatus from all of my astronomy stuff. Nevertheless, I’m back here on Steve’s Virtual Planet (SVP)!!

The really big news from here is that Fernbank Science Center and Observatory has reopened this summer and I am back on staff finally. So, I am really glad to be back on that scene and I’ll press on optimistically and start writing updates again.

Anyhow, another autumn and hopefully more stargazing (and moon gazing, too)! Certainly more blog entries with some new series planned. Also planned is an expansion of the section on archeo-astronomy and ethno-astronomy (I’ve been researching). And I hope for a revival of an older blog I had elsewhere on Space Weather and Solar Dynamics. That will be a future focus here at SVP.

Stay tuned and check back now and then!

Clear skies! (hopefully)

Steve

Solar Cycle 25

February 1st, 2021

If you appreciate some nice sunshine, you might also be interested in how our solar system’s central star behaves over the short term. We refer to these solar cycles to describe the periodic and repeating characteristics of our sun. The changes taking place in our sun repeat over time in a roughly 11 year cycle. Hence, the term.

These cycles have have been tracked for over 400 years, ever since the early Galilean days of the Scientific Revolution. We are now in Solar Cycle 25 and the current activity of our sun is under close and detailed scrutiny. Using a fleet of satellites and solar telescopes, we watch our closest star like a hawk, in every wavelength available.

Tune in to NASA’s Space Weather monitoring site and spaceweather.com for day-to-day (literally!) updates on the fascinating life of basic, run-o’-the-mill star in our very neighborhood.

And keep on eye on Steve’s Virtual Planet for future articles on Solar Dynamics such as this trip down memory lane that links to details about the 1859 Carrington Event.

Keep shinin’!!

First published Feb 1 , 2021 Updated Sep 23, 2024

SVC Tip #6 - Preferential treatment!

March 7th, 2020

As you may have figured out by now, I have been using Sky View Cafe for quite a while. Occasionally, I find something new (or quirky) so I thought I would bring a few things to your attention.

First, I like to set the calendar tab as my default view since I want check the moon phase and to choose the day first anyhow. This can easily be done using the blue button up on the right hand corner marked “More …“. When you click it, you get … more (of course), including a set of “preferences”, Just select the little gear icon and click. The second field allows you to set the Default view. Easy.

Next, I found a couple of quirks, one being that even though there seems to be some printer settings I have had no luck with any printing feature at all. So, you may have to look for other tools for this. Finally, even though the built-in Help is really good, you may need help finding it. The help link up in the right hand pane seems broken. So, instead, use the Help ? link up in the very top center or the one in the More … button. Viola! More easy!

I hope you are enjoying SVC as much as I am. If so, check out the other tips here SVC Tip #1 & SVC Tip #2 & SVC Tip #3, SVC Tip #4 and Tip #5.

Moon tools Pt 1 (The Intro)

December 16th, 2019

I’m a tool kinda guy. You know .. Swiss Army knife, a good flashlight, some vice grips, and, of course, a good astronomy app. Web based tools and apps for astronomy and stargazing are really the good stuff. This series is going to delve into various tools I’ve found on the web that help understand our moon better. This is part one, which, implies additional parts, theoretically. So, we’ll see how my research goes and how many tools we find.

Bar none, my favorite web site is still Sky View Cafe (SVC). You can see some of my other posts with details on the features, but my main tip here is to set your SVC startup view to be the calendar instead of the default Sky view. This is easy to do using the “More…” button up in the right corner.  Click on more and then on Preferences. Change the second setting value to Calendar and then click OK. This will set the applet to go to the calendar whenever it starts. From here, the moon phases are in full display with a graphic for each day.

In one of my previous postings, I featured an animation to show the Moon orbiting the Earth. This is a great applet from The University of Nebraska that has three different views of the effect of lunar phases from Earth’s perspective. At the same website, I also found a really useful animation that shows how the effect of the moon’s gravity and our proximity to the sun sets up the tides.

See how far you get with these suggestions. You can even howl if you like!!

Magnitude? Yes! (apparently)

April 1st, 2019

Yes, indeed! Apparently! That’s how we see a star’s brightness form our perspective here on Earth. We use the term “magnitude” to describe the brightness of a star. We call the measurement of the brightness from Earth the “apparent magnitude“. The effect of this apparent brightness leads us to the more exacting method of using a numbered scale to quantify what we see. And this scale goes all the way back to the days of ancient Greece and is credited to a very clever mathematician named Hipparchus.

Hipparchus came up with a six level scale based on naked eye brightness that is still largely the same today. In this scale, the number 1 is given to the brightest stars, with a gradual decrease in brightness shown with a higher number from 2 to 6. Yes, the number gets higher as the stars gets dimmer. It’s a purely arbitrary system that has been the convention since about 150 BC.

When you use a typical sky map or star chart, look for the legend that shows a row of different diameter dots with a set of numbers on them. SkyMap uses a scale from -1 to 4 for its range. Other maps sometimes extend the range down to 6 or 7.

In one of my earlier posts, I examined several properties of stars such as mass and size. I will leave that line of research to you but it does have some relation to the topic at hand. However, from a star gazer’s perspective, we don’t have to delve too deep into astrophysics to work with this brightness scale. The value for apparent magnitude is found in star charts and tables of the stars as well. In some cases it is otherwise listed as “visual magnitude”, which means the same thing.

In any case, stellar brightness from -1 down to about 4 is the typical range in the suburbs. If you’re out in the country and have a really dark site, you will likely get down to around 6 magnitude, perhaps even to 6.5. And don’t forget to get your eyes adapted to the darker conditions for a better experience looking for these dimmer objects.

Stellar size and magnitude

March 14th, 2019

A while ago, I got a great question from one of my students in the Emory class - what does a star’s size got to do with its magnitude? And as she later explained, the words “size” and “magnitude” mean almost the same thing. They are similar, in our common usage, however, we talking specifically about their use in astronomy. It was clear this was a question more about semantics.

So I decided to dig further to come up with a better distinction between these two terms. But I have to start first with a third word, at the risk of further tangling this whole response. That word is mass. When we talk about stars, we start with mass. Stuff. What stars are made of, mostly hydrogen as it turns out.

The terms magnitude and size differ from the term mass. They are interrelated to some degree but in a straightforward linear way. But we always start with mass when considering a star’s properties and then go from there.

Astronomical magnitude, in the sense of what we see, actually refers to apparent magnitude. It is a measurement of the “apparent” brightness of the star as seen from Earth.In the days of the famous Greek astronomer, magnitude meant “bigness”. However, by the mid-nineteenth century it was determined that stars were so far away that no accurate measurement could be made of any starts size.

Sometimes the word mass is interchanged with size. But mass doesn’t always translate directly to the physical size of a star. Our sun, for example, is slowly loosing mass over it’s lifetime but once it nears the end of its life and becomes a red giant, it will be much larger in terms of its physical size, namely its diameter.

There is far too much to say about stars in this blog from the point of view of astrophysics, but if you wish indulge try any of these web pages below for further reading.

List of stellar angular diameters

Universetoday: Size-of-Stars

ClassZone: A Stars Size

Stellar Mass

Astronomical Magnitude

Back for another year!

January 2nd, 2019

Welcome all to a new year and a new perspective. I feel inspired to move forward and to share my passion for astronomy with the outside world again for another year. There is much to revel in this coming year including the lunar eclipse on January 20! Check my next post for details. I hope to get some of my astro projects up and running, especially with my research on ethnoastronomy and archeoastronomy.

I also plan (again) to take this astronomy blog site to the next level in the coming months. I’ll be focused on completing the series on naked eye lunar observing and moon tools. I am also gathering some external online content on Solar Dynamics and Space Weather as a bonus, ya know, in my spare time. Stick around and watch this space for more stuff soon.

In any case, here is wishing you Clear Skies!

SVC Tip #5 - New Features

September 4th, 2018

Here’s another update in the series on using Sky View Cafe (SVC) and some details on the recent upgrade of this tool. Kerry Shetline has released the latest upgrade as of July 2017 with a slightly different look but it replaces the legacy Java version. There have been some refinements but it’s still the very familiar tool compared to the old one. The current version as of this writing is 1.4.14.

Java is not used any longer (yay!) so this means you won’t have those annoying instances of the tool just dying because a new security fix is needed.

There is an extensive help page but use the link within the “More …” button. Most things are fairly intuitive but there are likely things you don’t catch without a lot of trial and error.

Have a great time with SVC and check out the other tips here SVC Tip #1 & SVC Tip #2 & SVC Tip #3 & SVC Tip #4

Binocular Lunar Observing Pt 2

November 30th, 2017

In this post, we’ll continue the discussion of naked eye targets on our Moon. In the first post, we looked at some of the larger mare that present themselves during the week from new moon to 1st quarter. Let’s continue to “follow the terminator” and look for some more challenging objects to be found during the week up to 1st Qtr. We’ll use some of the so called “Pickering Dozen” to add to the hunt. I’ll call them “P12″ for short.

When the moon is at First Qtr (ie. illuminated “half way” on the right side), there are fewer of the prominent craters that appear later on. However, if you have located Mare Serenitatis and Mare Tranquillitatis, you can use these to find some more challenging mountains and regions on their edges. Between these two large features is a thinning kind of peninsula known as the Plinius Region. This is number 6 in the P12 list and named for the 41km diameter crater in its vicinity, Plinius. The crater is quite prominent and is paired up with a group of riles directly north of it called Rimae Linius.  You should be able to make out this feature to the left of the field at the juncture of both of these large features.

Number 7 of the P12 is immediately to the left, Mare Vaporum, The Sea of Vapors. At first quarter, this feature will be just to the right of the terminator just above the equator. It’s a smaller mare that looks a bit like an extension of Serenitatis to the south west.  That will be our reference point next time when we hike the Apennine Mountains near where the Apollo 15 mission landed!

Updated Sep 2, 2024

Binocular Lunar Observing Pt 1

October 14th, 2017

This is the first of several posts that discuss naked eye targets on our Moon. Instead of an overall geographical approach, I’ll proceed chronologically and “follow the terminator“, the shadow line that progresses across the moon’s surface as the phases advance.

For some easy targets, why not start with the Lunar Mare (maria is singular), those dark and typically large areas on the lunar surface. Before the time of Galileo, most people thought these dark areas were “seas”, hence the name. Now we know they are large flat (dry) plains of fairly smooth basalt that formed 3-4 billion years ago from early volcanic activity.

It’s best to get a small moon map in front of you so you can get oriented. The are downloadable ones like this one from S&T with a printable map on page 10 or this image with different sizes for different screens.

With map in front of you, work from the right back towards the left. This is the way the moon will be revealed as the phases progress from New Moon to Full Moon. It is also the first half of the moon’s full cycle that is visible in the evening. The first obvious object you can see even within the first week is Mare Crisium (Crises). As the nights pass, you will then see more of the Mare (The Sea of ..) - Fecunditatis (Fertitility), Tranquillitatis (Tranquility), Serenitatis (Serenity). By the time of the First Quarter, you will be able to see all of those features.

In the next post, we’ll look for some more challenging objects to be found during the week up to 1st Qtr.

Updated Sep 2, 2024