Classical Music Little-Known Favorites

I’ve been seriously listening to classical music—both through live performance and recordings—for nearly 50 years, and am always surprised to find that I still discover or am introduced to works that are new to me and extraordinarily moving. “How can I have gone so many years without discovering this?” I often ask myself when I hear such a piece. Often, these “new” works are by well-known composers, but sometimes they are by composers I have never heard of. And, of course, some of them are new works by living composers.

For example, in 2017, I created a continuously-updated blog entry for “Symphonies by Women” because I was embarrassed to admit I couldn’t name a single one off the top of my head. Well, as you can see there are hundreds, and some of the few I have had the privilege to hear are really good.

There is an enormous amount of unknown music out there, and if only 1% of this unknown music is first-rate, then there must be hundreds of composers and thousands of works that deserve more attention. In France, Thanh-Tâm Le, who has recently helped me so much with this list of symphonies by women, has compiled a larger list of almost 18,000 symphonies by both men and women, and that is only symphonies!

Do you have some favorite classical works (both new and old) that you only know through a live performance or a non-commercial recording? Do you have some favorite works on vinyl or CD that are not currently available on CD? I know I do.

I’ve created a discussion group on groups.io called Classical Music Little-Known Favorites where I hope you and others will post audio files, YouTube videos, etc., of little-known works that you are enamored of. My hope for this group is that music lovers all around the world will join and present new and neglected works for us to enjoy and champion. Please join and spread the word!

The Early Radio Universe

As the expanding universe cooled, the first neutral1 hydrogen atoms formed about 380,000 years after the Big Bang (ABB), and most of the hydrogen in the universe remained neutral until the first stars began forming at least 65 million years ABB.

The period of time from 380,000 to 65 million years or so ABB is referred to as the “dark ages” since at the beginning of this period the cosmic background radiation from the Big Bang had redshifted from visible light to infrared so the universe was truly dark (in visible light) until the first stars began to form at the end of this period.

All the while, neutral hydrogen atoms occasionally undergo a “spin-flip” transition where the electron transitions from the higher-energy hyperfine level of the ground state to the lower-energy hyperfine level, and a microwave photon of wavelength 21.1061140542 cm and frequency 1420.4057517667 MHz is emitted.

Throughout the dark ages, the 21 cm emission line was being emitted by the abundant neutral hydrogen throughout the universe, but as the universe continued to expand the amount of cosmological redshift between the time of emission and the present day has been constantly changing. The longer ago the 21 cm emission occurred, the greater the redshift to longer wavelengths. We thus have a great way to map the universe during this entire epoch by looking at the “spectrum” of redshifts of this particular spectral line.

380,000 and 65 million years ABB correspond to a cosmological redshift (z) of 1,081 and 40, respectively. We can calculate what the observed wavelength and frequency of the 21 cm line would be for the beginning and end of the dark ages.

\lambda _{obs} = (z+1)\cdot \lambda_{emit}


The observed wavelength (λobs) for the 21 cm line (λemit) at redshift (z) of 1,081 using the above equation gives us 22,836.8 cm or 228.4 meters.

\nu = \frac{c}{\lambda }


That gives us a frequency (ν) of 1.3 MHz (using the equation above), where the speed of light c = 299,792,458 meters per second.

So a 21 cm line emitted 380,000 years ABB will be observed to have a wavelength of 228.4 m and a frequency of 1.3 MHz.

Using the same equations, we find that a 21 cm line emitted 65 Myr ABB will be observed to have a wavelength of 8.7 m and a frequency of 34.7 MHz.

We thus will be quite interested in taking a detailed look at radio waves in the entire frequency range 1.3 – 34.7 MHz, with corresponding wavelengths from 228.4 m down to 8.7 m.2

The interference from the Earth’s ionosphere and the ever-increasing cacophony of humanity’s radio transmissions makes observing these faint radio signals all but impossible from anywhere on or near the Earth. Radio astronomers and observational cosmologists are planning to locate radio telescopes on the far side of the Moon—both on the surface and in orbit above it—where the entire mass of the Moon will effectively block all terrestrial radio interference. There we will finally hear the radio whispers of matter before the first stars formed.

1 By “neutral” we mean hydrogen atoms where the electron has not been ionized and resides in the ground state—not an excited state.

2 Incidentally, the 2.7 K cosmic microwave background radiation which is the “afterglow” of the Big Bang itself at the beginning of the dark ages (380,000 years ABB), peaks at a frequency between 160 and 280 GHz and a wavelength around 1 – 2 mm. So this is a much higher frequency and shorter wavelength than the redshifted 21 cm emissions we are proposing to observe here.

References

Ananthaswamy, Anil, “The View from the Far Side of the Moon”, Scientific American, April 2021, pp. 60-63. https://www.scientificamerican.com/article/telescopes-on-far-side-of-the-moon-could-illuminate-the-cosmic-dark-ages1/

Burns, Jack O., et al., “Global 21-cm Cosmology from the Farside of the Moon”, https://arxiv.org/ftp/arxiv/papers/2103/2103.05085.pdf

Koopmans, Léon, et al., “Peering into the Dark (Ages) with Low-Frequency Space Interferometers”, https://arxiv.org/ftp/arxiv/papers/1908/1908.04296.pdf

Ned Wright’s Javascript Cosmology Calculator, http://www.astro.ucla.edu/~wright/CosmoCalc.html

Classical Music Link List – Arizona, New Mexico, West Texas

Here is a list of all things classical-music-related in Arizona, New Mexico, and West Texas. If you have additional links to add or see an existing link that needs to be changed or removed, please post a comment!

The two abiding interests in my life have been astronomy and classical music. I guess you could call me a professional listener, although I do have a pretty decent tenor voice and would love to sing in a secular mixed choir again. I have aspirations of hosting my own classical music program at a public radio station, or at least providing recordings and commentary. I served several years on the board of the Ames International Orchestra Festival Association (AIOFA), including two terms as board president. It was a great experience bringing fine orchestras from all over the world to C.Y. Stephens Auditorium in Ames, Iowa and hosting them during their stay. I love symphony orchestras (chamber music, too!), and would be very happy to serve in a similar capacity during my active retirement years. Or volunteering at a university music department that has a symphony orchestra. While living in Ames, I had the opportunity to attend many wonderful faculty and student recitals.

I have family in West Texas, so am looking to relocate to be closer to them. Would love to connect with the classical music scene somewhere in this tri-state area, so if you know of any good volunteer opportunities, please let me know!

Video Meteors 2020 – II

During the second half of 2020, I serendipitously captured six meteors on my telescope’s 17 x 11 arcminute video field of view while observing potential asteroid occultation events. I used the method described in There’s a Meteor in My Image to determine the radiant for each meteor. Here they are.

Sporadic meteor 8 Jul 2020 UT; Field location TYC 7379-00569-1 in Scorpius
Each frame is an exposure of 0.13s (meteor is at left side of field)

A sporadic meteor is any meteor that does not come from a known radiant.

Probable sporadic meteor 22 Aug 2020 UT; Field location UCAC4 394-071682 in Serpens
Each frame is an exposure of 0.13s ; possibly a Perseid (meteor from upper right to lower left)
Probable sporadic meteor 29 Aug 2020 UT; Field location UCAC4 601-019523 in Auriga
Each frame is an exposure of 0.27s ; possibly a Perseid (meteor from upper right to lower left)
Orionid 11 Oct 2020 UT; Field location TYC 1337-01489-1 in Gemini; very fast!
Each frame is an exposure of 0.13s ; (meteor at upper right)
Sporadic meteor 14 Nov 2020 UT; Field location UCAC4 559-043312 in Gemini
Each frame is an exposure of 0.27s (meteor at upper right)
Probable Leonid 5 Dec 2020 UT; Field location UCAC4 410-001419 in Cetus
Each frame is an exposure of 0.13s ; (meteor along upper part of field)

None of these meteors were particularly bright, unfortunately, so you may want to use the full-screen button at the lower-right-hand corner of each video to see them well.

References

International Meteor Organization, 2o2o Meteor Shower Calendar, Jürgen Rendtel, ed. https://www.imo.net/files/meteor-shower/cal2020.pdf.

Space Records

Russian cosmonaut Valeri Polyakov, M.D. (1942-) holds the record for the longest spaceflight duration. During 1994-1995, he spent 437.8 contiguous days in orbit, almost all of them aboard the Mir space station.

The largest number of people in space at the same time was thirteen, and this has happened four times.

The fastest humans have ever traveled (relative to Earth) occurred on May 26, 1969 when the Apollo 10 crew (Thomas Stafford, John Young, and Eugene Cernan) reached a speed of 24,791 mph—just 0.0037% the speed of light.

Both Jerry Ross and Franklin Chang Díaz hold the record for the most spaceflights. Both astronauts have gone into space seven times. Jerry Ross (STS-61-B, STS-27, STS-37, STS-55, STS-74, STS-88, STS-110) between November 26, 1985 and April 19, 2002 (Space Shuttle Atlantis: 5, Columbia: 1, Endeavour: 1), and Franklin Chang Díaz (STS-61-C, STS-34, STS-46, STS-60, STS-75, STS-91, STS-111) between January 12, 1986 and June 19, 2002 (Space Shuttle Columbia: 2, Atlantis: 2, Discovery: 2, Endeavour: 1). Both astronauts were mission specialists in the NASA Astronaut Group 9, announced May 29, 1980.

The farthest humans have ever been from Earth occurred at 0:21 UT on April 15, 1970 when the crippled Apollo 13 spacecraft (Jim Lovell, Fred Haise, and Jack Swigert) executed a free-return trajectory to Earth. They were furthest from Earth above the lunar farside, 158 miles above the surface and 248,655 miles from Earth.

The youngest person ever to fly in space was Gherman Titov who was 25 years old during his solo Vostok 2 spaceflight on August 6, 1961. He was the second person to orbit the Earth.

The oldest person ever to fly in space was John Glenn who was 77 years old during his second spaceflight aboard the Space Shuttle Discovery STS-95 from October 29, 1998 to November 7, 1998. He was the first American to orbit the Earth in 1962.

The longest spacewalk occurred on March 11, 2001 when James Voss and Susan Helms were outside the Space Shuttle Discovery (STS-102) and the International Space Station for 8 hours and 56 minutes.

The longest moonwalk occurred on December 12-13, 1972 when Apollo 17 astronauts Eugene Cernan and Harrison Schmitt spent 7 hours and 37 minutes outside the lunar module on their second of three lunar excursions. All were longer than 7 hours. This was the final Apollo mission, and Gene Cernan, who died in 2017, is still the last person to walk on the surface of the Moon.

Shostakovich Piano Concertos

I’d like to introduce you to another fine classical music recording I’ve recently discovered, but first a little editorializing about classical recordings in general.

I hope the day never comes when physical media in the form of compact discs (or something similar) is completely replaced by digital downloads or streaming. The booklet enclosed with physical media always provides useful and often enlightening information about the music, and there’s artistry on the front and back covers. Having been in COVID-19 lockdown for nearly a year now, I yearn for real human interaction without technology instead of “virtual everything”. And I say that as a person who has made his career as a computer programmer. What does that have to do with music on a CD? Well, perhaps I’ve digressed, but let me just say a recording is a poor substitute for a live performance, and a digital file is a poor substitute for a CD. Happily, I have read recently that classical music is keeping the CD alive as popular music largely goes the way of the computer file. As for CD packaging, I much prefer a well-made jewel case (with a hub whose teeth don’t break off easily) over the cardboard digipak that is seeing more frequent use, including the Shostakovich disc I will be briefly discussing here.

I much prefer discs that feature works of just one composer. Not only are they more easily filed and retrieved, but, more importantly, they often introduce you to some lesser-known works of a composer. Something I have learned over my many years of listening to classical music recordings is that there are many first-rate lesser-known works of composers, both famous and not-so-famous. There is a lot of great music out there, waiting to be discovered and enjoyed, even after a lifetime of listening!

This disc featuring Russian pianist Anna Vinnitskaya (who now lives in Germany) is one such happy occasion. It features the two piano concertos of Dmitri Shostakovich (himself a fine pianist), plus two of his lesser-known works for two pianos (joined here by Ivan Rudin), Concertino for Two Pianos, op. 94, and Tarantella for Two Pianos, both of which were unknown to me. An all-Shostakovich disc!

Alpha Classics 203

This disc is a delight from beginning to end. Anna Vinnitskaya plays Shostakovich as well as anyone I have heard, with great intensity, energy, and precision during the rhythmic passages, and with great beauty and sensitivity during the legato passages. The Kremerata Baltica is really outstanding in the two piano concertos, as is the quality of the recording. The latter is much above average, I would say, perfectly balanced and articulated. Vinnitskaya herself conducts the orchestra from the piano in the Concerto for Piano, Trumpet and Strings, op. 35, where she is joined by a fine trumpet soloist, Tobias Willmer. Omer Meir Wellber skillfully conducts the orchestra in the Concerto for Piano and Orchestra, op. 102, and the Kremerata Baltica is joined by the Winds of the Staatskapelle Dresden in a perfect union and performance.

Anna Vinnitskaya grew up with the music of Shostakovich in her household, and developed an early and deep appreciation of his music and it shows throughout this recording. She performed his Second Piano Concerto for the first time at the age of eleven, and now at age 37, I have no doubt she is one of the finest performers of the piano music of Shostakovich in the world today. I hope I will have the opportunity to hear her play either of the Shostakovich piano concertos in the concert hall one day soon. Or any other piano works by Shostakovich, for that matter!


One thing I have become acutely aware of after decades of listening to classical music is the enormous difference there can be between live performances or recordings of the same work. Tempo can be one obvious difference. I tend not to like music that is on the fast end of the tempo continuum for a given work—I like to “savor” the notes. But anything as complex and nuanced as an orchestral palette can lend itself to many different interpretations. Yes, the notes are the same, but how a piece is played can make the difference between enthusiasm for the work or complete indifference.

Supernovae in the Milky Way

The first recorded supernova in our Milky Way galaxy (or anywhere else, for that matter) was seen to blaze forth in the constellation Centaurus by astute Chinese astronomers in 185 AD. Including that one, only seven confirmed supernovae have been observed in our Milky Way galaxy, though thousands are discovered each year in other galaxies.

Supernova light reached Earth in AD 185, 393, 1006, 1054, 1181, 1572, and 1604. All seven of these events occurred before the invention of the telescope. Are we overdue for another supernova? Well, given this ridiculously small sample, we can endeavor to do some simple “statistics”. The shortest recorded interval between two Milky Way supernovae was 32 years between 1572 and 1604. The longest interval has been 613 years, between the supernovae of 393 and 1006 (assuming none went unnoticed). On average then (such as it is), we “should” have seen a Milky Way supernova around 1841, and using the longest interval of 613 years, we might be expecting one by the year 2217. Undoubtedly, some supernovae in the Milky Way have escaped detection because they lay behind thick interstellar clouds.

The big mystery to me is why are there no recorded supernova events prior to 185 AD? The earliest extant records of astronomical events go back at least as far as 2316 BC (a comet in the constellation Crater was recorded by Chinese astronomers), but in the intervening 2,500 years there has been no mention of anything that could be attributed to a supernova. Or has there? Some writings before and after 185 AD suggest possible supernovae, but until a supernova remnant is identified, we need to look for other explanations.

Here follows a table of the known observed Milky Way supernovae. Of course, other supernova remnants have been discovered in our Milky Way galaxy, but no record has yet been discovered describing these events. Many of them predate recorded history.

In the table below, you’ll note that these supernovae tend to lie close to the galactic plane (galactic latitude b = 0°)—not at all surprising considering that’s where most of the stars are.

Milky Way Supernovae confirmed to have been observed

Some Early Piano Music by Robert Schumann

Naïve V 5364

I discovered the music of Johannes Brahms before that of Robert Schumann, but I revere the latter composer now as well. Knowing much of the music of both, there is no question that Robert Schumann had a huge influence on Brahms. Both wrote four symphonies, all eight of which are favorites of mine.

But here we turn our attention to some of the early piano music of Robert Schumann, completed when Schumann was in his 20s, before he was finally able to marry Clara Wieck, and before his first symphony.

These are performances of considerable beauty, passion, and sensitivity by French pianist Lise de la Salle. I highly recommend this CD (Naïve V 5364). The recording is excellent, and De la Salle seems to have an innate understanding of this music and its often rapidly changing moods, a delight throughout.

The works performed are Scenes from Childhood, op. 15; Abegg Variations, op. 1; and Fantasie in C Major, op. 17.

There are thirteen pieces in Scenes from Childhood. The most famous of these is No. 7 Träumerei (Dreaming), but I also especially like No. 1 (Of foreign lands and peoples) and No. 2 (A curious story).

  1. Of foreign lands and peoples
  2. A curious story
  3. Blind man’s buff
  4. Pleading child
  5. Happy enough
  6. An important event
  7. Dreaming
  8. At the fireside
  9. Knight of the hobby-horse
  10. Almost too serious
  11. Frightening
  12. Child falling asleep
  13. The poet speaks

This is followed by the Schumann’s first published work, the Abegg Variations, op. 1.

The disc concludes with the three-movement work, Fantasie in C Major, op. 17, arguably Schumann’s piano masterpiece, and a real tour de force in this performance by Lise de la Salle. When he wrote this piece, Schumann was already beginning to suffer from a mental disorder that would tragically claim his life only 20 years later—an illness with a physical origin that no doubt today could be easily cured.

For an excellent introduction to Robert Schumann and his wife, Clara Wieck Schumann—a piano virtuoso, composer, and teacher of considerable talent—I wholeheartedly recommend the eight-part video course from Robert Greenberg, “Great Masters: Robert and Clara Schumann – Their Lives and Music” (The Great Courses, Course No. 759).

Even though it is a highly fictionalized account, I would also recommend the 1947 movie Song of Love, starring the incomparable Katharine Hepburn as Clara Wieck Schumann, Paul Henreid as Robert Schumann, and Robert Walker as Johannes Brahms.

Zodiacal Light 2021

In 2021, the best dates and times for observing the zodiacal light are listed in the calendar below. The sky must be very clear with little or no light pollution. The specific times listed are for Dodgeville, Wisconsin (42° 58′ N, 90° 08′ W).

Here’s a nicely-formatted printable PDF file of the zodiacal light calendar:

January 2021
SUN MON TUE WED THU FRI SAT
          1 2
3 4 5 6 7 8 9
10 11 12 13 14 15 16
17 18 19 20 21 22 23
24 25 26 27 28 29 30
Zodiacal Light 6:49 – 7:26 p.m. West
31
Zodiacal Light 6:50 – 7:50 p.m. West
           

February 2021
SUN MON TUE WED THU FRI SAT
  1
Zodiacal Light 6:51 – 7:51 p.m. West
2
Zodiacal Light 6:52 – 7:52 p.m. West
3
Zodiacal Light 6:53 – 7:53 p.m. West
4
Zodiacal Light 6:54 – 7:54 p.m. West
5
Zodiacal Light 6:56 – 7:56 p.m. West
6
Zodiacal Light 6:57 – 7:57 p.m. West
7
Zodiacal Light 6:58 – 7:58 p.m. West
8
Zodiacal Light 6:59 – 7:59 p.m. West
9
Zodiacal Light 7:00 – 8:00 p.m. West
10
Zodiacal Light 7:02 – 8:02 p.m. West
11
Zodiacal Light 7:03 – 8:03 p.m. West
12
Zodiacal Light 7:04 – 8:04 p.m. West
13
14 15 16 17 18 19 20
21 22 23 24 25 26 27
28
Zodiacal Light 7:23 – 7:36 p.m. West
           

March 2021
SUN MON TUE WED THU FRI SAT
  1
Zodiacal Light 7:25 – 8:25 p.m. West
2
Zodiacal Light 7:26 – 8:26 p.m. West
3
Zodiacal Light 7:27 – 8:27 p.m. West
4
Zodiacal Light 7:28 – 8:28 p.m. West
5
Zodiacal Light 7:29 – 8:29 p.m. West
6
Zodiacal Light 7:31 – 8:31 p.m. West
7
Zodiacal Light 7:32 – 8:32 p.m. West
8
Zodiacal Light 7:33 – 8:33 p.m. West
9
Zodiacal Light 7:34 – 8:34 p.m. West
10
Zodiacal Light 7:36 – 8:36 p.m. West
11
Zodiacal Light 7:37 – 8:37 p.m. West
12
Zodiacal Light 7:38 – 8:38 p.m. West
13
Zodiacal Light 7:40 – 8:40 p.m. West
14
Zodiacal Light 8:41 – 9:41 p.m. West
15 16 17 18 19 20
21 22 23 24 25 26 27
28 29 30
Zodiacal Light 9:03 – 10:03 p.m. West
31
Zodiacal Light 9:04 – 10:04 p.m. West
     

April 2021
SUN MON TUE WED THU FRI SAT
        1
Zodiacal Light 9:05 – 10:05 p.m. West
2
Zodiacal Light 9:07 – 10:07 p.m. West
3
Zodiacal Light 9:08 – 10:08 p.m. West
4
Zodiacal Light 9:10 – 10:10 p.m. West
5
Zodiacal Light 9:11 – 10:11 p.m. West
6
Zodiacal Light 9:13 – 10:13 p.m. West
7
Zodiacal Light 9:14 – 10:14 p.m. West
8
Zodiacal Light 9:16 – 10:16 p.m. West
9
Zodiacal Light 9:17 – 10:17 p.m. West
10
Zodiacal Light 9:19 – 10:19 p.m. West
11
Zodiacal Light 9:20 – 10:20 p.m. West
12
Zodiacal Light 9:22 – 10:22 p.m. West
13
Zodiacal Light 9:24 – 10:24 p.m. West
14 15 16 17
18 19 20 21 22 23 24
25 26 27 28 29 30  

May 2021
SUN MON TUE WED THU FRI SAT
            1
2 3 4 5 6 7 8
9 10 11 12 13 14 15
16 17 18 19 20 21 22
23 24 25 26 27 28 29
30 31          

June 2021
SUN MON TUE WED THU FRI SAT
    1 2 3 4 5
6 7 8 9 10 11 12
13 14 15 16 17 18 19
20 21 22 23 24 25 26
27 28 29 30      

July 2021
SUN MON TUE WED THU FRI SAT
        1 2 3
4 5 6 7 8 9 10
11 12 13 14 15 16 17
18 19 20 21 22 23 24
25 26 27 28 29 30 31

August 2021
SUN MON TUE WED THU FRI SAT
1 2 3 4 5 6 7
8 9 10 11 12 13 14
15 16 17 18 19 20 21
22 23 24 25 26 27 28
29 30 31        

September 2021
SUN MON TUE WED THU FRI SAT
      1 2 3 4
5 6
Zodiacal Light 3:52 – 4:52 a.m. East
7
Zodiacal Light 3:53 – 4:53 a.m. East
8
Zodiacal Light 3:54 – 4:54 a.m. East
9
Zodiacal Light 3:56 – 4:56 a.m. East
10
Zodiacal Light 3:57 – 4:57 a.m. East
11
Zodiacal Light 3:58 – 4:58 a.m. East
12
Zodiacal Light 4:00 – 5:00 a.m. East
13
Zodiacal Light 4:01 – 5:01 a.m. East
14
Zodiacal Light 4:02 – 5:02 a.m. East
15
Zodiacal Light 4:04 – 5:04 a.m. East
16
Zodiacal Light 4:05 – 5:05 a.m. East
17
Zodiacal Light 4:06 – 5:06 a.m. East
18
Zodiacal Light 4:08 – 5:08 a.m. East
19
Zodiacal Light 4:59 – 5:09 a.m. East
20 21 22 23 24 25
26 27 28 29 30    

October 2021
SUN MON TUE WED THU FRI SAT
          1 2
3 4 5
Zodiacal Light 4:28 – 5:28 a.m. East
6
Zodiacal Light 4:30 – 5:30 a.m. East
7
Zodiacal Light 4:31 – 5:31 a.m. East
8
Zodiacal Light 4:32 – 5:32 a.m. East
9
Zodiacal Light 4:33 – 5:33 a.m. East
10
Zodiacal Light 4:34 – 5:34 a.m. East
11
Zodiacal Light 4:35 – 5:35 a.m. East
12
Zodiacal Light 4:37 – 5:37 a.m. East
13
Zodiacal Light 4:38 – 5:38 a.m. East
14
Zodiacal Light 4:39 – 5:39 a.m. East
15
Zodiacal Light 4:40 – 5:40 a.m. East
16
Zodiacal Light 4:41 – 5:41 a.m. East
17
Zodiacal Light 4:42 – 5:42 a.m. East
18
Zodiacal Light 5:03 – 5:43 a.m. East
19 20 21 22 23
24 25 26 27 28 29 30
31            

November 2021
SUN MON TUE WED THU FRI SAT
  1 2 3 4
Zodiacal Light 5:03 – 6:03 a.m. East
5
Zodiacal Light 5:04 – 6:04 a.m. East
6
Zodiacal Light 5:05 – 6:05 a.m. East
7
Zodiacal Light 4:06 – 5:06 a.m. East
8
Zodiacal Light 4:07 – 5:07 a.m. East
9
Zodiacal Light 4:08 – 5:08 a.m. East
10
Zodiacal Light 4:09 – 5:09 a.m. East
11
Zodiacal Light 4:10 – 5:10 a.m. East
12
Zodiacal Light 4:12 – 5:12 a.m. East
13
Zodiacal Light 4:13 – 5:13 a.m. East
14
Zodiacal Light 4:14 – 5:14 a.m. East
15
Zodiacal Light 4:15 – 5:15 a.m. East
16
Zodiacal Light 4:16 – 5:16 a.m. East
17
Zodiacal Light 5:06 – 5:17 a.m. East
18 19 20
21 22 23 24 25 26 27
28 29 30        

December 2021
SUN MON TUE WED THU FRI SAT
      1 2 3 4
5 6 7 8 9 10 11
12 13 14 15 16 17 18
19 20 21 22 23 24 25
26 27 28 29 30 31  

The best nights to observe the zodiacal light at mid-northern latitudes occur when the ecliptic plane intersects the horizon at an angle of 60° or steeper. The dates above were chosen on that basis, with the Sun at least 18° below the horizon and the Moon below the horizon being used to calculate the times. An interval of time of one hour either before morning twilight or after evening twilight was chosen arbitrarily because it is the “best one hour” for observing the zodiacal light. The zodiacal light cone will be brightest and will reach highest above the horizon when the Sun is 18° below the horizon (astronomical twilight), but no less.

If you are interested in calculating the angle the ecliptic makes with your horizon for any date and time, you can use the following formula:

\cos I = \cos \varepsilon \sin \phi-\sin \varepsilon \cos \phi \sin \theta

where I is the angle between the ecliptic and the horizon, ε is  the obliquity of the ecliptic, φ is the latitude of the observer, and θ is the local sidereal time (the right ascension of objects on the observer's meridian at the time of observation).

Here’s a SAS program I wrote to do these calculations:

References
Meeus, J. Astronomical Algorithms. 2nd ed., Willmann-Bell, 1998, p. 99.

Meteor Shower Calendar 2021

Here’s our meteor shower calendar for 2021.  It is sourced from the IMO’s Working List of Visual Meteor Showers (https://www.imo.net/files/meteor-shower/cal2021.pdf, Table 5, p. 25).

Each meteor shower is identified using its three-character IAU meteor shower code.  Codes are bold on the date of maximum, and one day either side of maximum.

Here’s a printable PDF file of the meteor shower calendar shown below:

Happy meteor watching!

January 2021
SUN MON TUE WED THU FRI SAT
          1
DLM QUA
2
DLM QUA
3
DLM QUA
4
DLM QUA
5
DLM QUA
6
DLM QUA
7
DLM QUA
8
DLM QUA
9
DLM QUA
10
DLM QUA GUM
11
DLM QUA GUM
12
DLM QUA GUM
13
DLM GUM
14
DLM GUM
15
DLM GUM
16
DLM GUM
17
DLM GUM
18
DLM GUM
19
DLM GUM
20
DLM GUM
21
DLM GUM
22
DLM GUM
23
DLM
24
DLM
25
DLM
26
DLM
27
DLM
28
DLM
29
DLM
30
DLM
31
DLM ACE
           
February 2021
SUN MON TUE WED THU FRI SAT
  1
DLM ACE
2
DLM ACE
3
DLM ACE
4
DLM ACE
5
ACE
6
ACE
7
ACE
8
ACE
9
ACE
10
ACE
11
ACE
12
ACE
13
ACE
14
ACE
15
ACE
16
ACE
17
ACE
18
ACE
19
ACE
20
ACE
21 22 23 24 25
GNO
26
GNO
27
GNO
28
GNO
           
March 2021
SUN MON TUE WED THU FRI SAT
  1
GNO
2
GNO
3
GNO
4
GNO
5
GNO
6
GNO
7
GNO
8
GNO
9
GNO
10
GNO
11
GNO
12
GNO
13
GNO
14
GNO
15
GNO
16
GNO
17
GNO
18
GNO
19
GNO
20
GNO
21
GNO
22
GNO
23
GNO
24
GNO
25
GNO
26
GNO
27
GNO
28
GNO
29 30 31      
April 2021
SUN MON TUE WED THU FRI SAT
        1 2 3
4 5 6 7 8 9 10
11 12 13 14
LYR
15
PPU LYR
16
PPU LYR
17
PPU LYR
18
PPU LYR
19
ETA PPU LYR
20
ETA PPU LYR
21
ETA PPU LYR
22
ETA PPU LYR
23
ETA PPU LYR
24
ETA PPU LYR
25
ETA PPU LYR
26
ETA PPU LYR
27
ETA PPU LYR
28
ETA PPU LYR
29
ETA LYR
30
ETA LYR
 
May 2021
SUN MON TUE WED THU FRI SAT
            1
ETA
2
ETA
3
ELY ETA
4
ELY ETA
5
ELY ETA
6
ELY ETA
7
ELY ETA
8
ELY ETA
9
ELY ETA
10
ELY ETA
11
ELY ETA
12
ELY ETA
13
ELY ETA
14
ARI ELY ETA
15
ARI ETA
16
ARI ETA
17
ARI ETA
18
ARI ETA
19
ARI ETA
20
ARI ETA
21
ARI ETA
22
ARI ETA
23
ARI ETA
24
ARI ETA
25
ARI ETA
26
ARI ETA
27
ARI ETA
28
ARI ETA
29
ARI
30
ARI
31
ARI
         
June 2021
SUN MON TUE WED THU FRI SAT
    1
ARI
2
ARI
3
ARI
4
ARI
5
ARI
6
ARI
7
ARI
8
ARI
9
ARI
10
ARI
11
ARI
12
ARI
13
ARI
14
ARI
15
ARI
16
ARI
17
ARI
18
ARI
19
ARI
20
ARI
21
ARI
22
JBO ARI
23
JBO ARI
24
JBO ARI
25
JBO
26
JBO
27
JBO
28
JBO
29
JBO
30
JBO
     
July 2021
SUN MON TUE WED THU FRI SAT
        1
JBO
2
JBO
3
CAP
4
CAP
5
CAP
6
CAP
7
CAP
8
CAP
9
CAP
10
CAP
11
CAP
12
CAP SDA
13
CAP SDA
14
CAP SDA
15
CAP SDA PAU
16
CAP SDA PAU
17
PER CAP SDA PAU
18
PER CAP SDA PAU
19
PER CAP SDA PAU
20
PER CAP SDA PAU
21
PER CAP SDA PAU
22
PER CAP SDA PAU
23
PER CAP SDA PAU
24
PER CAP SDA PAU
25
PER CAP SDA PAU
26
PER CAP SDA PAU
27
PER CAP SDA PAU
28
PER CAP SDA PAU
29
PER CAP SDA PAU
30
PER CAP SDA PAU
31
PER CAP SDA PAU
August 2021
SUN MON TUE WED THU FRI SAT
1
PER CAP SDA PAU
2
PER CAP SDA PAU
3
KCG PER CAP SDA PAU
4
KCG PER CAP SDA PAU
5
KCG PER CAP SDA PAU
6
KCG PER CAP SDA PAU
7
KCG PER CAP SDA PAU
8
KCG PER CAP SDA PAU
9
KCG PER CAP SDA PAU
10
KCG PER CAP SDA PAU
11
KCG PER CAP SDA
12
KCG PER CAP SDA
13
KCG PER CAP SDA
14
KCG PER CAP SDA
15
KCG PER CAP SDA
16
KCG PER SDA
17
KCG PER SDA
18
KCG PER SDA
19
KCG PER SDA
20
KCG PER SDA
21
KCG PER SDA
22
KCG PER SDA
23
KCG PER SDA
24
KCG PER
25
KCG
26 27 28
AUR
29
AUR
30
AUR
31
AUR
       
September 2021
SUN MON TUE WED THU FRI SAT
      1
AUR
2
AUR
3
AUR
4
AUR
5
SPE AUR
6
SPE
7
SPE
8
SPE
9
DSX SPE
10
STA DSX SPE
11
STA DSX SPE
12
STA DSX SPE
13
STA DSX SPE
14
STA DSX SPE
15
STA DSX SPE
16
STA DSX SPE
17
STA DSX SPE
18
STA DSX SPE
19
STA DSX SPE
20
STA DSX SPE
21
STA DSX SPE
22
STA DSX
23
STA DSX
24
STA DSX
25
STA DSX
26
STA DSX
27
STA DSX
28
STA DSX
29
STA DSX
30
STA DSX
   
October 2021
SUN MON TUE WED THU FRI SAT
          1
STA DSX
2
ORI STA DSX
3
ORI STA DSX
4
ORI STA OCT DSX
5
ORI STA OCT DSX
6
ORI STA DRA OCT DSX
7
ORI STA DRA DSX
8
ORI STA DRA DSX
9
ORI STA DRA DSX
10
ORI DAU STA DRA
11
ORI DAU STA
12
ORI DAU STA
13
ORI DAU STA
14
ORI EGE DAU STA
15
ORI EGE DAU STA
16
ORI EGE DAU STA
17
ORI EGE DAU STA
18
ORI EGE DAU STA
19
LMI ORI EGE STA
20
NTA LMI ORI EGE STA
21
NTA LMI ORI EGE STA
22
NTA LMI ORI EGE STA
23
NTA LMI ORI EGE STA
24
NTA LMI ORI EGE STA
25
NTA LMI ORI EGE STA
26
NTA LMI ORI EGE STA
27
NTA LMI ORI EGE STA
28
NTA ORI STA
29
NTA ORI STA
30
NTA ORI STA
31
NTA ORI STA
           
November 2021
SUN MON TUE WED THU FRI SAT
  1
NTA ORI STA
2
NTA ORI STA
3
NTA ORI STA
4
NTA ORI STA
5
NTA ORI STA
6
LEO NTA ORI STA
7
LEO NTA ORI STA
8
LEO NTA STA
9
LEO NTA STA
10
LEO NTA STA
11
LEO NTA STA
12
LEO NTA STA
13
NOO LEO NTA STA
14
NOO LEO NTA STA
15
NOO AMO LEO NTA STA
16
NOO AMO LEO NTA STA
17
NOO AMO LEO NTA STA
18
NOO AMO LEO NTA STA
19
NOO AMO LEO NTA STA
20
NOO AMO LEO NTA STA
21
NOO AMO LEO NTA
22
NOO AMO LEO NTA
23
NOO AMO LEO NTA
24
NOO AMO LEO NTA
25
NOO AMO LEO NTA
26
NOO LEO NTA
27
NOO LEO NTA
28
PHO NOO LEO NTA
29
PHO NOO LEO NTA
30
PHO NOO LEO NTA
       
December 2021
SUN MON TUE WED THU FRI SAT
      1
PUP PHO NOO NTA
2
PUP PHO NOO NTA
3
HYD PUP PHO NOO NTA
4
GEM HYD PUP PHO NOO NTA
5
DLM GEM HYD MON PUP PHO NOO NTA
6
DLM GEM HYD MON PUP PHO NOO NTA
7
DLM GEM HYD MON PUP PHO NTA
8
DLM GEM HYD MON PUP PHO NTA
9
DLM GEM HYD MON PUP PHO NTA
10
DLM GEM HYD MON PUP NTA
11
DLM GEM HYD MON PUP
12
DLM COM GEM HYD MON PUP
13
DLM COM GEM HYD MON PUP
14
DLM COM GEM HYD MON PUP
15
DLM COM GEM HYD MON PUP
16
DLM COM GEM HYD MON
17
DLM URS COM GEM HYD MON
18
DLM URS COM GEM HYD MON
19
DLM URS COM GEM HYD MON
20
DLM URS COM GEM HYD MON
21
DLM URS COM
22
DLM URS COM
23
DLM URS COM
24
DLM URS
25
DLM URS
26
DLM URS
27
DLM
28
DLM QUA
29
DLM QUA
30
DLM QUA
31
DLM QUA