The NASA All Sky Fireball Network is already detecting the first meteors of this year’s Perseid meteor shower! The meteor shower peaks on the night of August 12 as the Earth passes through the dustiest debris of comet Swift-Tuttle’s trails.
On July 26, 2023, the NASA All Sky Fireball Network detected the first Perseid meteor of the year. (NASA/All Sky Fireball Network)
The Perseid meteor shower is often considered to be the best meteor shower of the year due to its high rates and pleasant late-summer temperatures. Unlike last year’s shower coinciding with the full moon, this year’s moon will be a waning crescent, allowing even some of the fainter meteors to be seen.
So, how many can you see?
“People in the U.S. can reasonably expect to see around 40 Perseids in the hour just before dawn on the peak nights. That’s about one every couple of minutes, which is not bad,” said Bill Cooke, who leads NASA’s Meteoroid Environment Office. “However, we are assuming you are out in the country, well away from cities and suburbs.”
The brighter skies of suburban areas greatly reduce the rates, with 10 or fewer expected in an hour.
You can see the Perseid meteor shower best in the Northern Hemisphere. All you need to catch the show is a clear sky, darkness, and a bit of patience. You don’t need to look in any particular direction; meteors can generally be seen all over the sky.
This diagram, based on data from the NASA Fireball Network, shows the change in the direction of the Perseid radiant with time. This is caused by Earth’s motion about the Sun, causing the radiant to appear to “drift” with respect to the background stars. (Danielle Moser, NASA Meteoroid Environment Office)
The Perseids appear to radiate from a point in the constellation Perseus, and each meteor has a similar orbit. Meteor showers take their name from the location of their point of origin, or what is known as the radiant.
On June 1, 1993, the orbiter Discovery is shown here being rolled into the Vehicle Assembly Building (VAB) for mating with the external tank and twin solid rocket boosters. At the time, Discovery was being prepared for mission STS-51, targeted for a mid-July liftoff. (NASA/JSC)
Fun fact: The Perseid meteor shower is the only meteor shower to delay a Space Shuttle launch. In 1993, the NASA – STS-51 launch was delayed due to concerns about the Perseid meteor shower activity being forecast to be extremely heavy, increasing the chance that a spacecraft in Earth orbit could be damaged by a piece of the debris.
By Lauren Perkins NASA Marshall Space Flight Center
Fireworks won’t be the only bright objects lighting the sky this month. The next full moon will appear on the morning of Monday, July 3, although it will seem full for up to three days.
The nearly full moon rises over the city of New Orleans on Tuesday evening, May 25, 2021. Photo credit: NASA/ Michael DeMocker
The July full moon is also called the “Full Buck Moon,” according to the Farmers’ Almanac, as this is the time of year when male deer antlers are in full growth. Alternatively, the Haida and Tlingit Indian Tribes of Alaska referred to the July full moon as the “Salmon Moon,” as it was a time of significant salmon migration. Perhaps you have heard the phrase describing corn fields as growing to “knee-high by fourth of July?” The Eastern Band of Cherokee Indians would refer to the July full Moon as the “Corn in Tassel Month,” due to the growth cycle of the crop.
This will be the first full Moon of the summer season and the first full Moon after the Summer Solstice. Lunar enthusiasts will have two super opportunities for full-Moon gazing in August – the Sturgeon Supermoon and the Blue Supermoon.
As the moon transitions to third quarter, Earth’s next brightest neighbor, Venus, will reach its greatest illuminated extent. Around July 7, Venus will reach apparent magnitude – 4.6. For reference, a full Moon, the second brightest celestial object after the Sun, has an apparent magnitude up to –12.6 and the faintest star you can see with your eye has a magnitude of +7.2.
The northern hemisphere is displayed in this global view of the surface of Venus as seen by NASA Magellan spacecraft. Image Credit: NASA/JPL
Finally, wrap up the month by sharing some lunar love on International Moon Day July 20 next time on Watch the Skies!
Sky enthusiasts, start off summer by witnessing two extraordinary celestial events in June – the Full Strawberry Moon and the summer solstice. These events hold both historical and cultural significance.
The Moon rises as a Metrorail car crosses the Potomac river in Washington 50 years to the day after astronauts Neil Armstrong, Michael Collins, and Buzz Aldrin launched on Apollo 11, the first mission to land astronauts on the Moon, Tuesday, July 16, 2019. Photo Credit: NASA/Bill Ingalls
The Full Strawberry Moon, depending on one’s time zone, will illuminate the night sky on June 3. Although the exact moment of full moon occurs when the Moon is opposite the Earth from the Sun, its full appearance will extend for about a day before and after the event. Remember to bring binoculars or a telescope to see all of the details of the Moon’s craters and other lunar features.
The name “Full Strawberry Moon” originated from the Algonquin tribes in the northeastern United States. This full moon occurred during the month of June when strawberries were ripening and ready to be harvested. The name “Strawberry Moon” has been passed down through generations and continues to be used by many today.
Diagram of the Earth’s alignment with the Sun for the June and December solstices. (NASA)
Later in the month on June 21, the summer solstice will mark the beginning of the astronomical summer and the longest day in the Northern Hemisphere, and the start of winter and the shortest day in the Southern Hemisphere. This change in season is due to the 23.5-degree tilt of the Earth’s axis compared to its orbit around the sun, allowing the most direct sunlight to reach the Northern Hemisphere this month.
Throughout history, this celestial event has played a crucial role in various civilizations, shaping their calendars, traditions, and agricultural practices. Farmers would rely on the June Solstice to determine when to plant and harvest crops. The solstice’s timing influenced the development of many calendars, such as the ancient Roman calendar and the modern Gregorian calendar.
May is a great month for stargazing with a host of celestial events happening in the morning and evening skies.
On May 17, a slim crescent moon will rise about an hour before the Sun. From much of the United States and Canada, you’ll be able to see Jupiter appearing very close to the Moon. In some southern U.S. states, Jupiter will pass behind the Moon as the pair rises in morning twilight. From western states, Jupiter will be behind the Moon, in occultation, as the duo rise. Jupiter will start to emerge from behind the Moon as the Sun comes up. To observe this event, you’ll need a clear view of the horizon, and a pair of binoculars will be essential as many locations in the U.S. will be in daylight during this occultation.
Astronaut Scott Kelly observes three planets and Earth’s Moon in an impressive display while conducting long-duration space flight research aboard the International Space Station. The image reveals Earth’s Moon, Venus, Jupiter, and Earth’s crescent, arranged from bottom to top. Credit: NASA/Scott Kelly
Following sunset from May 22 through 24, you’ll be able to witness a close grouping of the Moon, Venus, and Mars in the western sky. The Moon will sit between the two planets on the 23rd. Venus has been rising higher in the sky each evening for the past few months, but in May, it’ll reach its highest point in the western sky.
For those stargazing from the Southern Hemisphere, there are some key differences in the night sky compared to the Northern Hemisphere. For instance, there’s no counterpart to the North Star in the Southern Hemisphere, and the seasonal star patterns that a northern observer are familiar with appear flipped upside down when viewed in southern skies.
Some celestial objects are only visible from Earth’s Southern Hemisphere, such as central portions of our Milky Way galaxy, left, plus the two Magellanic Clouds above and to the left of the observatory dome, as shown in this photo taken at Cerro Paranal in Chile’s Atacama Desert. Credits: ESO / Y. Beletsky
Two entire galaxies, the large and small Magellanic Clouds, can be easily observed in the southern sky with the unaided eye. These are dwarf galaxies that orbit our own Milky Way galaxy.
If you are interested in what else is in the sky for May, check out the latest “What’s Up” video from Jet Propulsion Laboratory:
Enjoy these stellar spectacles as you watch the skies!
The eta Aquariid meteor shower is active throughout April and May, peaking in the pre-dawn hours of May 5. This year could be particularly impressive as an outburst year with 120-160 meteors per hour expected.
“A meteor shower is like a normal rain shower, with 50-60 meteors per hour,” said Bill Cooke, lead of NASA’s Meteoroid Environments Office at the agency’s Marshall Space Flight Center in Huntsville, Alabama. “An outburst is like a thunderstorm, with greater than normal meteor activity expected. A meteor storm is like a tornado, where meteor rates are over one thousand per hour.”
Despite the full moon lighting up the sky and washing out the faint meteors, this year’s eta Aquariid meteor shower is not one to miss. In terms of producing fireballs, NASA camera data places it #6 among meteor showers. These bright fireballs are caused by Earth running into a dense stream of debris from Comet Halley, a lot of which was ejected more than 3,000 years ago. Moving at 148,000 mph, some of these fireballs leave glowing “trains” in their wake that last for several seconds to minutes.
C-141 Kuiper Airborne Imagery of Comet Halley (New Zealand Expedition) PHOTO CREDIT Photo taken with equipment designed, mounted on the headring and operated by the Charleston (South Carolina) County School District CAN DO Project;
How to View
The eta Aquariid meteor shower is viewable in both the Northern and Southern hemispheres, with higher rates of visibility to observers in the Southern Hemisphere. This is due to the radiant’s location in the constellation of Aquarius. Meteors will be observable after midnight, but the peak times are 3-4 a.m. until dawn.
Regardless of your geographic location, you’ll want to find an area well away from city lights for best viewing. Give yourself about 30 minutes in the dark for your eyes to adapt – this means not looking at your phone. Look AWAY from the moon and take in as much sky as possible.
An image of an Eta Aquarid meteor from the NASA All Sky Fireball Network station in Tullahoma, Tennessee in May, 2013.
The next major meteor showers will be the Perseids in August, and the sister show to the eta Aquariids, the Orionids in October.
But there’s plenty more skygazing to do this month. Check out What’s Up in May from NASA Jet Propulsion Laboratory.
This year’s Lyrid meteor shower will peak in the predawn hours of April 23. On average, the shower can produce up to 15 meteors per hour under ideal viewing conditions. The Lyrids occur every year in mid-April, when Earth crosses the trail of debris left by the Comet C/1861 G1 Thatcher. These bits of comet burn up when they hit Earth’s atmosphere and produce this shower of shooting stars. The shower gets its name from the constellation Lyra, the point in the sky where the meteors appear to originate. Unlike the Perseids or Geminids, the Lyrids are not known for bright fireballs. What makes them special is their unpredictability.
Lyrid Meteors from the Constellation Lyra – Image Credit & Copyright: Petr Horálek
The first record of the Lyrid meteor shower dates back 2,700 years, making it one of the oldest in history. Researchers looking though old records have found descriptions of major Lyrid outbursts. For example, a notation made by the French bishop Gregory of Tours in April of 582 A.D. states, “At Soissons, we see the sky on fire.” There was also a Lyrid outburst visible over the United States in 1803. An article in the Virginia Gazette and General Advertiser describes the shower: “From one until three, those starry meteors seemed to fall from every point in the heavens, in such numbers as to resemble a shower of sky rockets.” The last Lyrid outburst was in 1982, when 75 meteors per hour were recorded by observers in Florida.
The common theme here is that Lyrid outbursts are surprises. Unlike some other showers, meteor researchers aren’t able to predict Lyrid outbursts as well. That’s why it is important to make observations each year so that models of its activity can be improved.
How can you best observe the Lyrids? After 10:30 p.m. local time on the night of April 22, find a dark place away from city lights with open sky free of clouds and look straight up. It will take about 30 minutes for your eyes to get acclimated to the dark. Don’t look at your cell phone – the bright light from its screen will interrupt your night vision. You will begin to see Lyrids, and as the night progresses the meteors will appear more often, reaching 10 to 15 per hour in the pre-dawn hours of the 23rd. You can see Lyrids on the night before and after the peak, but the rates will be lower, maybe five per hour or so.
The cosmos’ annual gift to sky watchers, the Geminids Meteor shower, will peak on Dec. 13-14 this year.
During peak activity and perfect weather conditions, which are rare, the Geminids produce approximately 100-150 meteors per hour for viewing. However, this year a waning gibbous moon will make it harder to view most of the shower, resulting in only 30-40 visible meteors per hour at the peak in the Northern Hemisphere, depending on sky conditions. But the Geminids are so bright that this should still be a good show.
Bill Cooke, lead of NASA’s Meteoroid Environments Office at Marshall Space Flight Center in Huntsville, Alabama, suggests sitting in the shade of a house or tree while also maintaining a view of the open sky to alleviate moonlight interference.
The meteor shower is coined the Geminids because the meteors appear to radiate from the constellation Gemini. According to Cooke, meteors close to the radiant have very short trails and are easily missed, so observers should avoid looking at that constellation. However, tracing a meteor backwards to the constellation Gemini can determine if you caught a Geminid (other weaker showers occur at the same time).
Gemini does not appear very high above the horizon in the Southern Hemisphere, resulting in viewers only seeing approximately 25% of the rates seen in the Northern Hemisphere, which is between 7-10 meteors per hour. Sky watchers from the Southern Hemisphere are encouraged to find areas with minimal light pollution and look to the northern sky to improve their viewing opportunities.
Over 100 meteors are recorded in this composite image taken during the peak of the Geminid meteor shower in 2014. Credit: Jacobs Space Exploration Group/ESSCA
The Geminids start around 9 or 10 p.m. CST on Dec. 13, making it a great viewing opportunity for any viewers who cannot be awake during later hours of the night. The shower will peak at 6 a.m. CST on Dec. 14, but the best rates will be seen earlier around 2 a.m. local time. You can still view Geminids just before or after this date, but the last opportunity is on Dec. 17 – when a dedicated observer could possibly spot one or two on that night.
For prime viewing, find an area away from city and streetlights, bundle up for winter weather conditions, bring a blanket or sleeping bag for extra comfort, lie flat on your back with your feet facing south, and look up. Practice patience because it will take approximately 30 minutes for your eyes to fully adjust and see the meteors. Refrain from looking at your cell phone or other bright objects to keep your eyes adjusted.
The show will last for most of the night, so you have multiple opportunities to spot the brilliant streaks of light across our sky.
So where does this magnificent shower come from? Meteors are fragments and particles that burn up as they enter Earth’s atmosphere at high speed, and they usually originate from comets.
The Geminid shower originates from the debris of 3200 Phaethon an asteroid first discovered on Oct. 11, 1983, using the Infrared Astronomical Satellite. Phaethon orbits the Sun every 1.4 years, and every year Earth passes through its trail of debris, resulting in the Geminids Shower.
Phaethon is the first asteroid to be associated with a meteor shower, but astronomers debate its exact classification and origins. Phaethon lacks an icy shell (the staple characteristic of a comet), but some consider it a “dead comet” – suggesting it once had an icy shell that melted away. Other astronomers call it a “rock comet” because Phaethon passes very close to the Sun during its orbit, which theoretically results in heating and cracking that creates debris and dust. The bottom line is Phaethon’s exact origins are still a mystery, but we do know it’s the Geminids parent body.
Geminids travel 78,000 miles per hour, over 40 times faster than a speeding bullet, but it is highly unlikely that meteors will reach the ground – most Geminids burn up at altitudes between 45 to 55 miles.
An info graphic based on 2019’s meteor camera data for the Geminids. Credit: NASA
In addition to sky watching opportunities, meteor videos recorded by the NASA All Sky Fireball Network are available each morning to identify Geminids in these videos – just look for events labeled “GEM.”
And, if you want to know what else is in the sky for December, check out the video below from Jet Propulsion Laboratory’s monthly “What’s Up” video series:
For the second time in 2022, stargazers will have the opportunity to view a total lunar eclipse on Nov. 8. At least a portion of the phenomenon will be visible throughout eastern Asia, Australia, the Pacific, and North America. The previous total lunar eclipse happened in May.
According to Alphonse Sterling, astrophysicist from NASA’s Marshall Space Flight Center in Huntsville, Alabama, total lunar eclipses occur approximately once every 1.5 years on average. While the Moon has been providing generous eclipse viewing opportunities this year, viewers should take advantage of November’s eclipse because the next total lunar eclipse will not occur until 2025.
The Flower Moon lunar eclipse over NASA’s Michoud Assembly Facility in New Orleans is shown from the initial partial eclipse to totality in a composite of seven images shot on Sunday, May 15, 2022. Image credit: NASA/Michael DeMocker
A total lunar eclipse occurs when Earth casts a complete shadow – called an umbra – over the Moon. Earth’s shadow is categorized into two parts: the umbra, the innermost part of the shadow where direct light from the Sun is completely blocked, and the penumbra, the outermost part of the shadow where the light is partially blocked.
During a total lunar eclipse, the Moon and the Sun are on opposite sides of Earth. Many people wonder why lunar eclipses don’t happen every month given the Moon completes an orbit around Earth every 27 days. The reason is because the Moon’s orbit around Earth is tilted relative to Earth’s orbit around the Sun, so the Moon often passes above or below Earth’s shadow. Lunar eclipses are only possible when the orbits align so that the Moon is directly behind Earth relative to the Sun.
For North America the action will start in the early hours of the morning on Nov. 8. The partial eclipse will begin at 3:09 a.m. CST, with totality beginning at 4:16 a.m. and ending at 5:42 a.m. Then, the partial phase will resume, lasting until 6:49 a.m. Those in the eastern part of the United States will miss most or all of the last partial phase because the Moon will set during totality or shortly after totality ends.
Another feature of a total lunar eclipse is the Moon’s red hue during totality. The red color occurs because of the refraction, filtering, and scattering of light by Earth’s atmosphere. The scattering is a phenomenon called Rayleigh scattering – named after the 19th-century British Physicist Lord Rayleigh.
Rayleigh scattering is also the reason for red sunrises and sunsets. Light from the Sun collides into the gases of Earth’s atmosphere and because of its shorter wavelength, blue light is filtered out, but red light is not easily scattered because of its longer wavelength. Some of that red light is refracted, or bent, as it passes through Earth’s atmosphere and ends up shining on the Moon with a ghostly red light. The degree of redness of a fully eclipsed Moon can be influenced by atmospheric conditions resulting from volcanic eruptions, fires, and dust storms.
A nearly total eclipse of November’s full “Beaver Moon” captured over the city of New Orleans before dawn on Nov. 19, 2021. The 97% eclipse clocked in at 3 hours, 28 minutes, and 24 seconds, making it the longest partial lunar eclipse in 580 years. Credits: NASA/Michoud Assembly Facility
But what does Earth look like from the Moon’s perspective during a lunar eclipse? According to Mitzi Adams, astrophysicist at Marshall, astronauts on the Moon during a total lunar eclipse would see a red ring around a silhouetted Earth. As NASA works to establish a permanent human presence on the Moon through the Artemis program, it’s fascinating to consider how Earthlings will experience astronomical events away from their home planet.
No special eye protection is needed for viewing a lunar eclipse, unlike solar eclipses (which occur during the daytime). While the lunar eclipse can be observed with the unaided eye, a pair of binoculars or a telescope can enhance the view.
Sterling says a fun activity for those who stargaze with family or friends is to discuss who notices the reddish hue of totality first and how it progresses throughout the eclipse.
Gain more understanding of lunar eclipses, learn about NASA’s observations of eclipses, and inspire young stargazers with activities and information.
Finally, if you want to know what else is happening as you watch the skies in November, check out Jet Propulsion Laboratory’s latest “What’s Up” video:
Complemented by cooler temperatures and falling leaves, the September equinox marks the beginning of the fall season for the Northern Hemisphere. This year’s autumnal equinox (for the Northern Hemisphere) or spring equinox (for the Southern Hemisphere) occurs on Sept. 22 at 8:04 p.m. CDT.
An illustration of the March (spring) and September (fall or autumn) equinoxes. During the equinoxes, both hemispheres receive nearly equal amounts of daylight. (Image not to scale) Credits: NASA/GSFC/Genna Duberstein
During an equinox the Sun shines directly over the equator resulting in nearly equal amounts of day and night throughout the world – except for the North and South Pole where the Sun approximately straddles the horizon for the entire day, according to Alphonse Sterling, an astrophysicist at NASA’s Marshall Space Flight Center in Huntsville, Alabama. Following the autumnal equinox, the Sun gradually continues to rise later and set earlier in the Northern Hemisphere – making the days shorter and the nightfall longer. The opposite is true in the Southern Hemisphere where the days begin to last longer.
Seasons are caused by Earth’s tilted axis which always points in the same direction. As Earth orbits around the Sun, the angle of sunlight that the Northern and Southern Hemispheres receive is different. “On the June solstice (summer) in the Northern Hemisphere, sunlight is more direct, so it warms the ground more efficiently,” said Mitzi Adams an Assistant Manager in the Heliophysics and Planetary Science Branch at Marshall. “In the Southern Hemisphere, sunlight is less direct (winter), which means that the ground is not heated as easily.”
A visual aid to better understand how the Earth’s tilted axis causes the different seasons throughout the year in the Northern and Southern Hemispheres. Credit: NASA/Space Place
Astronomical seasons are defined by the Earth’s journey around the Sun, while meteorological seasons are guided by annual temperature cycles. Meteorologists group the seasons into time periods that line up with the weather and monthly calendar: December through February is winter, March through May is spring, June through August is summer, and September through November is fall. Astronomical seasons are marked by the equinoxes and solstices that each happen twice a year. Solstices are when the Sun appears to reach the lowest or highest point in the sky all year; they mark the beginning of summer or winter. Solstices are commonly referred to as the longest (summer solstice) or shortest (winter solstice) day of the year.
The September equinox is a time that welcomes Earthlings to a new season. To those in the Northern Hemisphere, enjoy the beginning of milder weather and say hello to early sunsets and late sunrises.
Stargazers can expect excellent views of Jupiter the entire night of Monday, Sept. 26 when the giant planet reaches opposition. From the viewpoint of Earth’s surface, opposition happens when an astronomical object rises in the east as the Sun sets in the west, placing the object and the Sun on opposite sides of Earth.
Jupiter’s opposition occurs every 13 months, making the planet appear larger and brighter than any other time of the year. But that’s not all. Jupiter will also make its closest approach to Earth since 1963 – almost six decades ago! This happens because Earth and Jupiter do not orbit the Sun in perfect circles – meaning the planets will pass each other at different distances throughout the year. Jupiter’s closest approach to Earth rarely coincides with opposition, which means this year’s views will be extraordinary. At its closest approach, Jupiter will be approximately 367 million miles in distance from Earth, about the same distance it was in 1963. The massive planet is approximately 600 million miles away from Earth at its farthest point.
This photo of Jupiter, taken from the Hubble Space Telescope on June 27, 2019, features the Great Red Spot, a storm the size of Earth that has been raging for hundreds of years. Credits: NASA, ESA, A. Simon (Goddard Space Flight Center), and M.H. Wong (University of California, Berkeley)
“With good binoculars, the banding (at least the central band) and three or four of the Galilean satellites (moons) should be visible,” said Adam Kobelski, a research astrophysicist at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “It’s important to remember that Galileo observed these moons with 17th century optics. One of the key needs will be a stable mount for whatever system you use.”
Kobelski recommends a larger telescope to see Jupiter’s Great Red Spot and bands in more detail; a 4 inch-or-larger telescope and some filters in the green to blue range would enhance the visibility of these features.
According to Kobelski, an ideal viewing location will be at a high elevation in a dark and dry area.
“The views should be great for a few days before and after Sept. 26,” Kobelski said. “So, take advantage of good weather on either side of this date to take in the sight. Outside of the Moon, it should be one of the (if not the) brightest objects in the night sky.”
As the Moon rose over the Wasatch Mountains near Salt Lake City on Feb. 27, 2019, the planet Jupiter could be seen, along with three of its largest moons. Stargazers should have a similar view during Jupiter in Opposition on Monday, Sept. 26. Credits: NASA/Bill Dunford
Jupiter has 53 named moons, but scientists believe that 79 moons have been detected in total. The four largest moons, Io, Europa, Ganymede, and Callisto, are called the Galilean satellites. They are named after the man who first observed them in 1610, Galileo Galilei. In binoculars or a telescope, the Galilean satellites should appear as bright dots on either side of Jupiter during opposition.
NASA’s Juno spacecraft, which has been orbiting Jupiter for six years, is dedicated to exploring the planet and its moons. Juno began its journey in 2011 and reached Jupiter five years later. Since 2016, the spacecraft has provided incredible images and data about Jupiter’s lively atmosphere, interior structures, internal magnetic field, and magnetosphere.
Scientists believe studying Jupiter can lead to breakthrough discoveries about the formation of the solar system. Juno’s mission was recently extended until 2025 or until the end of the spacecraft’s life. Learn more about Juno.
The next major project for Jupiter exploration is the Europa Clipper. This spacecraft will explore Jupiter’s iconic moon, Europa, which is known for its icy shell and vast ocean that lies beneath its surface. NASA scientists aim to find whether Europa has conditions able to sustain life. Europa Clipper’s targeted launch is currently scheduled for no earlier than October 2024.
Learn more about the giant planet. And if you want to know what else is happening in the sky for September, check out Jet Propulsion Laboratory’s latest “What’s Up” video:
