In fact, this summer brings several red letter days in Red Planet exploration. Here are 10 things to know about the anniversary of the Curiosity landing—plus some other arrivals at Mars you may not know about.
This self-portrait of NASA's Curiosity Mars rover shows the vehicle at a drilled sample site called "Okoruso," on the "Naukluft Plateau" of lower Mount Sharp. The scene combines multiple images taken with the rover's Mars Hand Lens Imager (MAHLI) on May 11, 2016. Credit: NASA/JPL-CALTECH/MSSS
For Curiosity, landing on Mars meant slowing from about 13,000 MPH (21,000 KPH) to a full stop in just seven minutes. Engineers came up with an innovative--and bold--plan to make this happen, but no one could be 100% certain it would work. In this video, some of the Curiosity engineers who designed the entry, descent and landing system for the mission talk candidly about the challenges of Curiosity's final moments before touchdown in August 2012.
Relive the tension, and the celebration, of the night Curiosity landed on Mars. You can also simulate the entire landing process in 3-D on your own computer using NASA's free Eyes on the Solar System app.
What has Curiosity discovered during its roving so far? The key takeaway: the stark deserts of Gale Crater were once home to lakes and streams of liquid water, a place where life could potentially have thrived. Learn more about the mission's scientific findings.
Sometimes science can be beautiful, as pictures from Mars prove. You can peruse some of Curiosity's best shots. What's more, you can see the very latest images—often on the same day they're downlinked from Mars.
Have you ever wanted to try driving a Mars rover yourself? You can (virtually anyway). Try the Experience Curiosity app right in your web browser.
Maybe someday you'll be able to take a day hike across the Martian landscape. You can at least plan your route right now, using NASA's Mars Trek site. This interactive mapping tool lets you explore important Red Planet locations using actual terrain imagery from orbiting satellites. You can even retrace the real locations on Mars where the fictional astronaut Mark Watney traveled in "The Martian."
Curiosity stands (well, rolls) on the shoulders of giants. Several NASA missions blazed the trail for the current crop of robotic explorers. The first was Mariner 4, which is also celebrating an anniversary this summer. Mariner 4 was the first spacecraft to return photos of another planet from deep space when it flew by Mars on July 15, 1965. Mariner engineers were so impatient to see the first pictures it sent back, that they hand-colored a printout of raw numeric data sent by the spacecraft, in order to construct one of the first color images of Mars.
Another important pathfinder on Mars was...Mars Pathfinder. This mission just marked its 20th anniversary. To commemorate the first successful Mars rover, NASA created a new 360-degree VR panorama of its landing site you can view right in your browser.
The first spacecraft to make a successful landing on Mars was Viking 1, which touched down in the Chryse Planitia region on July 20, 1976. It worked for more than six years, performing the first Martian soil analysis using its robotic arm and an onbaord biological laboratory. While it found no conclusive evidence of life, Viking 1 did help us understand Mars as a planet with volcanic soil, a thin, dry carbon dioxide atmosphere and striking evidence for ancient river beds and vast flooding.
There is much more to come. The next Mars lander, InSight, is slated for launch next year. Ride along with NASA's ongoing adventures on the Red Planet at: mars.nasa.gov/mars-exploration/
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Big news for our Nancy Grace Roman Space Telescope! Thanks to some new “shades” – an infrared filter that will help us see longer wavelengths of light – the mission will be able to spot water ice on objects in the outer solar system, see deeper into clouds of gas and dust, and peer farther across space. We’re gearing up for some super exciting discoveries!
You probably know that our solar system includes planets, the Sun, and the asteroid belt in between Mars and Jupiter – but did you know there’s another ‘belt’ of small objects out past Neptune? It’s called the Kuiper belt, and it’s home to icy bodies that were left over from when our solar system formed.
A lot of the objects there are like cosmic fossils – they haven’t changed much since they formed billions of years ago. Using its new filter, Roman will be able to see how much water ice they have because the ice absorbs specific wavelengths of infrared light, providing a “fingerprint” of its presence. This will give us a window into the solar system’s early days.
Clouds of dust and gas drift throughout our galaxy, sometimes blocking our view of the stars behind them. It’s hard for visible light to penetrate this dusty haze because the particles are the same size or even larger than the light’s wavelength. Since infrared light travels in longer waves, it hardly notices the tiny particles and can pass more easily through dusty regions.
With Roman’s new filter, we’ll be able to see through much thicker dust clouds than we could have without the upgrade. It’ll be much easier to study the structure of our home galaxy, the Milky Way.
Roman’s expanded view will also help us learn more about brown dwarfs – objects that are more massive than planets, but not massive enough to light up like stars. The mission will find them near the heart of the galaxy, where stars explode more often.
These star explosions, called supernovae, are so extreme that they create and disperse new elements. So near the center of the galaxy, there should be higher amounts of elements that aren’t as common farther away, where supernovae don’t happen as often.
Astronomers think that may affect how stars and planets form. Using the new filter, Roman will probe the composition of brown dwarfs to help us understand more.
Roman’s upgraded filter will also help us see farther across space. As light travels through our expanding universe, its wavelength becomes stretched. The longer it travels before reaching us, the longer its wavelength becomes. Roman will be able to see so far back that we could glimpse some of the first stars and galaxies that ever formed. Their light will be so stretched that it will mostly arrive as infrared instead of visible light.
We’re still not sure how the very first galaxies formed because we’ve found so few of these super rare and faint beasts. But Roman will have such a big view of the universe and sharp enough vision that it could help us find a lot more of them. Then astronomers can zoom in on them with missions like our James Webb Space Telescope for a closer look.
Roman will help us explore these cosmic questions and many more! Learn more about the mission here: https://roman.gsfc.nasa.gov/
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As a child, Kate Rubins dreamed of being an astronaut and a scientist. During the past four months aboard the International Space Station, that dream came full circle. She became the first person to sequence DNA in space, among other research during her recent mission, adding to her already impressive experience. She holds a doctorate in molecular biology, and previously led a lab of 14 researchers studying viruses, including Ebola.
Here’s a look back at Rubins in her element, conducting research aboard your orbiting laboratory.
The U.S. national laboratory, called Destiny, is the primary research laboratory for U.S. payloads, supporting a wide range of experiments and studies contributing to health, safety, and quality of life for people all over the world.
Destiny houses the Microgravity Science Glovebox (MSG), in which Kate worked on the Heart Cells experiment.
Microbes that can cause illness could present problems for current and future long duration space missions.
Understanding what microbe communities thrive in space habitats could help researchers design antimicrobial technology. Here, Kate is sampling various surfaces of the Kibo module for the Microbe-IV investigation.
The Heart Cells investigation uses human skin cells that are induced to become stem cells, which can then differentiate into any type of cell.
Researchers forced the stem cells to grow into human heart cells, which Rubins cultured aboard the space station for one month.
Rubins described seeing the heart cells beat for the first time as “pretty amazing. First of all, there’s a few things that have made me gasp out loud up on board the [space] station. Seeing the planet was one of them, but I gotta say, getting these cells in focus and watching heart cells actually beat has been another pretty big one.”
The Hard to Wet Surfaces investigation from Eli Lilly, and sponsored by the Center for the Advancement of Science in Space (CASIS), looks at liquid-solid interactions and how certain pharmaceuticals dissolve, which may lead to more potent and effective medicines in space and on Earth.
Rubins set up vials into which she injected buffer solutions and then set up photography to track how tablets dissolved in the solution in microgravity.
Rubins assisted in the capture of the SpaceX Dragon cargo spacecraft in July. The ninth SpaceX resupply mission delivered more than two thousand pounds of science to the space station.
Biological samples and additional research were returned on the Dragon spacecraft more than a month later.
Science doesn’t just happen inside the space station. External Earth and space science hardware platforms are located at various places along the outside of the orbiting laboratory.
The Japanese Experiment Module airlock can be used to access the JEM Exposed Facility. Rubins installed the JEM ORU Transfer Interface (JOTI) on the JEM airlock sliding table used to install investigations on the exterior of the orbiting laboratory.
Rubins installed an optical diagnostic instrument in the Microgravity Science Glovebox (MSG) as part of the Selective Optical Diagnostics Instrument (SODI-DCMIX) investigation. Molecules in fluids and gases constantly move and collide.
When temperature differences cause that movement, called the Soret effect, scientists can track it by measuring changes in the temperature and movement of mass in the absence of gravity. Because the Soret effect occurs in underground oil reservoirs, the results of this investigation could help us better understand such reservoirs.
When Rubins’ expedition began, DNA had never been sequenced in space. Within just a few weeks, she and the Biomolecule Sequencer team had sequenced their one billionth “base” – the unit of DNA - aboard the orbiting laboratory.
The Biomolecule Sequencer investigation seeks to demonstrate that DNA sequencing in microgravity is possible, and adds to the suite of genomics capabilities aboard the space station.
The SPHERES-Slosh investigation examines the way liquids move inside containers in a microgravity environment. The phenomena and mechanics associated with such liquid movement are still not well understood and are very different than our common experiences with a cup of coffee on Earth.
Rockets deliver satellites to space using liquid fuels as a power source, and this investigation plans to improve our understanding of how propellants within rockets behave in order to increase the safety and efficiency of future vehicle designs. Rubins conducted a series of SPHERES-Slosh runs during her mission.
Precious science samples like blood, urine and saliva are collected from crew members throughout their missions aboard the orbiting laboratory.
They are stored in the Minus Eighty-Degree Laboratory Freezer for ISS (MELFI) until they are ready to return to Earth aboard a Soyuz or SpaceX Dragon vehicle.
Our WetLab-2 hardware system is bringing to the space station the technology to measure gene expression of biological specimens in space, and to transmit the results to researchers on Earth at the speed of light.
Rubins ran several WetLab-2 RNA SmartCycler sessions during her mission.
The Bigelow Expandable Activity Module (BEAM) is the first expandable habitat to be installed on the space station. It was expanded on May 28, 2016.
Expandable habitats are designed to take up less room on a spacecraft, but provide greater volume for living and working in space once expanded. Rubins conducted several evaluations inside BEAM, including air and surface sampling.
Airway Monitoring, an investigation from ESA (the European Space Agency), uses the U.S. airlock as a hypobaric facility for performing science. Utilizing the U.S. airlock allows unique opportunities for the study of gravity, ambient pressure interactions, and their effect on the human body.
This investigation studies the occurrence and indicators of airway inflammation in crew members, using ultra-sensitive gas analyzers to evaluate exhaled air. This could not only help in spaceflight diagnostics, but that also hold applications on earth within diagnostics of similar conditions, for example monitoring of asthma.
Fire behaves differently in space, where buoyant forces are removed. Studying combustion in microgravity can increase scientists’ fundamental understanding of the process, which could lead to improvement of fire detection and suppression systems in space and on Earth.
Many combustion experiments are performed in the Combustion Integration Rack (CIR) aboard the space station. Rubins replaced two Multi-user Droplet Combustion Apparatus (MDCA) Igniter Tips as part of the CIR igniter replacement operations.
Though Rubins is back on Earth, science aboard the space station continues, and innovative investigations that seek to benefit humans on Earth and further our exploration of the solar system are ongoing. Follow @ISS_Research to keep up with the science happening aboard your orbiting laboratory.
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Today is Small Business Saturday, which the U.S. Small Business Administration (SBA) recognizes as a day to celebrate and support small businesses and all they do for their communities.
Source: Techshot
We are proud to partner with small businesses across the country through NASA’s Small Business Innovative Research (SBIR) and Small Business Technology Transfer (STTR) programs, which have funded the research, development and demonstration of innovative space technologies since 1982. This year, we’ve awarded 571 SBIR/STTR contracts totaling nearly $180 million to companies who will support our future exploration:
Techshot, Inc. was selected to bioprint micro-organs in a zero-gravity environment for research and testing of organs-on-chip devices, which simulate the physiological functions of body organs at a miniature scale for health research without the need for expensive tests or live subjects.
CertainTech, Inc., with the George Washington University, will demonstrate an improved water recovery system for restoring nontoxic water from wastewater using nanotechnology.
Electrochem, Inc. was contracted to create a compact and lightweight regenerative fuel cell system that can store energy from an electrolyzer during the lunar day to be used for operations during the lunar night.
Source: Electrochem
Small businesses are also developing technologies for the Artemis missions to the Moon and for human and robotic exploration of Mars. As we prepare to land the first woman and next man on the Moon by 2024, these are just a few of the small businesses working with us to make it happen.
Masten Space Systems, Astrobotic and Tyvak Nano-Satellite Systems are three NASA SBIR/STTR alumni now eligible to bid on NASA delivery services to the lunar surface through Commercial Lunar Payload Services (CLPS) contracts. Other small businesses selected as CLPS providers include Ceres Robotics, Deep Space Systems, Intuitive Machines, Moon Express, and Orbit Beyond. Under the Artemis program, these companies could land robotic missions on the Moon to perform science experiments, test technologies and demonstrate capabilities to help the human exploration that will follow. The first delivery could be as early as July 2021.
One cornerstone of our return to the Moon is a small spaceship called Gateway that will orbit our nearest neighbor to provide more access to the lunar surface. SBIR/STTR alum Advanced Space Systems will develop a CubeSat that will test out the lunar orbit planned for Gateway, demonstrating how to enter into and operate in the unique orbit. The Cislunar Autonomous Positioning System Technology Operations and Navigation Experiment (CAPSTONE) could launch as early as December 2020.
We selected 14 companies as part of our Tipping Point solicitation, which fosters the development of critical, industry-led space capabilities for our future missions. These small businesses all proposed unique technologies that could benefit the Artemis program.
Many of these small businesses are also NASA SBIR/STTR alumni whose Tipping Point awards are related to their SBIR or STTR awards. For example, Infinity Fuel Cell and Hydrogen, Inc. (Infinity Fuel) will develop a power and energy product that could be used for lunar rovers, surface equipment, and habitats. This technology stems from a new type of fuel cell that Infinity Fuel developed with the help of NASA SBIR/STTR awards.
CU Aerospace and Astrobotic are also small businesses whose Tipping Point award can be traced back to technology developed through the NASA SBIR/STTR program. CU Aerospace will build a CubeSat with two different propulsion systems, which will offer high performance at a low cost, and Astrobotic will develop small rover “scouts” that can host payloads and interface with landers on the lunar surface.
This is just a handful of the small businesses supporting our journey back to the Moon and on to Mars, and just a taste of how they impact the economy and American innovation. We are grateful for the contributions that small businesses make—though they be but “small,” they are fierce.
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The Apollo 11 Command Module “Columbia” is hoisted onto its recovery ship the USS Hornet, following splashdown on July 24, 1969. Credit: NASA
Four days after their historic achievement, Apollo 11 astronauts Neil Armstrong, Buzz Aldrin and Michael Collins splashed down in the Pacific Ocean at 12:49 p.m. EDT, about 900 miles from Hawaii. The crew was recovered by the crew of the USS Hornet where President Richard Nixon was waiting to greet them.
Watch a replay of the original live broadcast of the recovery on NASA TV starting at 12:45 p.m. EDT.
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NASA astronauts Shannon Walker, Victor Glover, and Mike Hopkins, and JAXA (Japan Aerospace Exploration Agency) astronaut Soichi Noguchi embark on a historic mission on November 14, 2020 aboard the Crew Dragon. NASA’s Crew-1 mission marks the first certified crew rotation flight to the International Space Station. During their 6-month stay on orbit, these crew members will don their science caps and complete experiments in microgravity. Check out five out of this world experiments you can expect to see these space scientists working on during Expedition 64.
The Crew-1 astronauts will become space farmers with the responsibility of tending to the rad(ish) garden located in a facility known as the Advanced Plant Habitat (APH). Researchers are investigating radishes in the Plant Habitat-02 experiment as a candidate crop for spaceflight applications to supplement food sources for astronauts. Radishes have the benefits of high nutritional content and quick growth rates, making these veggies an intriguing option for future space farmers on longer missions to the Moon or Mars.
Microbes can seemingly do it all, including digging up the dirt (so to speak). The BioAsteroid investigation looks at the ability of bacteria to break down rock. Future space explorers could use this process for extracting elements from planetary surfaces and refining regolith, the type of soil found on the moon, into usable compounds. To sum it up, these microbial miners rock.
The iconic spacesuits used to walk on the moon and perform spacewalks on orbit are getting an upgrade. The next generation spacesuit, the Exploration Extravehicular Mobility Unit (xEMU), will be even cooler than before, both in looks and in terms of ability to regulate astronaut body temperature. The Spacesuit Evaporation Rejection Flight Experiment (SERFE) experiment is a technology demonstration being performed on station to look at the efficiency of multiple components in the xEMU responsible for thermal regulation, evaporation processes, and preventing corrosion of the spacesuits.
Crew-1 can expect to get a delivery of many types of chips during their mission. We aren’t referring to the chips you would find in your pantry. Rather, Tissue Chips in Space is an initiative sponsored by the National Institutes of Health to study 3D organ-like constructs on a small, compact devices in microgravity. Organ on a chip technology allows for the study of disease processes and potential therapeutics in a rapid manner. During Expedition 64, investigations utilizing organ on a chip technology will include studies on muscle loss, lung function, and the blood brain barrier – all on devices the size of a USB flashdrive.
Circadian rhythm, otherwise known as our "internal clock," dictates our sleep-wake cycles and influences cognition. Fruit flies are hitching a ride to the space station as the subjects of the Genes in Space-7 experiment, created by a team of high school students. These flies, more formally known as the Drosophila melanogaster, are a model organism, meaning that they are common subjects of scientific study. Understanding changes in the genetic material that influences circadian rhythm in microgravity can shed light on processes relevant to an astronaut’s brain function.
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For updates on other platforms, follow @ISS_Research, Space Station Research and Technology News, or our Facebook to keep up with the science happening aboard your orbiting laboratory, and step outside to see the space station passing over your town using Spot the Station.
Inside this metal box, it’s punishingly cold. The air is unbreathable. The pressure is so low, you’d inflate like a balloon. This metal chamber is essentially Mars in a box — or a near-perfect replica of the Martian environment. This box allows scientists to practice chemistry experiments on Earth before programming NASA’s Curiosity rover to carry them out on Mars. In some cases, scientists use this chamber to duplicate experiments from Mars to better understand the results. This is what’s happening today.
The ladder is set so an engineer can climb to the top of the chamber to drop in a pinch of lab-made Martian rock. A team of scientists is trying to duplicate one of Curiosity’s first experiments to settle some open questions about the origin of certain organic compounds the rover found in Gale Crater on Mars. Today’s sample will be dropped for chemical analysis into a tiny lab inside the chamber known as SAM, which stands for Sample Analysis at Mars. Another SAM lab is on Mars, inside the belly of Curiosity. The SAM lab analyzes rock and soil samples in search of organic matter, which on Earth is usually associated with life. Mars-in-a-box is kept at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
This is Goddard engineer Ariel Siguelnitzky. He is showing how far he has to drop the sample, from the top of the test chamber to the sample collection cup, a small capsule about half an inch (1 centimeter) tall (pictured right below). On Mars, there are no engineers like Siguelnitzky, so Curiosity’s arm drops soil and rock powder through small funnels on its deck. In the photo, Siguelnitzky’s right hand is pointing to a model of the tiny lab, which is about the size of a microwave. SAM will heat the soil to 1,800 degrees Fahrenheit (1,000 degrees Celsius) to extract the gases inside and reveal the chemical elements the soil is made of. It takes about 30 minutes for the oven to reach that super high temperature.
Each new sample is dropped into one of the white cups set into a carousel inside SAM. There are 74 tiny cups. Inside Curiosity’s SAM lab, the cups are made of quartz glass or metal. After a cup is filled, it’s lifted into an oven inside SAM for heating and analysis.
Amy McAdam, a NASA Goddard geochemist, hands Siguelnitzky the sample. Members of the SAM team made it in the lab using Earthly ingredients that duplicate Martian rock powder. The powder is wrapped in a nickel capsule (see photo below) to protect the sample cups so they can be reused many times. On Mars, there’s no nickel capsule around the sample, which means the sample cups there can’t be reused very much.
SAM needs as little as 45 milligrams of soil or rock powder to reveal the secrets locked in minerals and organic matter on the surface of Mars and in its atmosphere. That’s smaller than a baby aspirin!
Siguelnitzky has pressurized the chamber – raised the air pressure to match that of Earth – in order to open the hatch on top of the Mars box.
Now, he will carefully insert the sample into SAM through one of the two small openings below the hatch. They’re about 1.5 inches (3.8 centimeters) across, the same as on Curiosity. Siguelnitzky will use a special tool to carefully insert the sample capsule about two feet down to the sample cup in the carousel.
Sample drop.
NASA Goddard scientist Samuel Teinturier is reviewing the chemical data, shown in the graphs, coming in from SAM inside Mars-in-a-box. He’s looking to see if the lab-made rock powder shows similar chemical signals to those seen during an earlier experiment on Mars.
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Our solar system is huge, so let us break it down for you. Here are 5 things you should know this week:
1. From Pluto, with Love
Last Valentine’s Day, no one had even seen Pluto’s most famous feature, the heart-shaped Sputnik Planum. These days, the New Horizons spacecraft is sending more and more pictures back to Earth from its Pluto flyby last July. We received new ones almost on a weekly basis. For the latest love from the outer solar system, go HERE.
2. Saturn’s Rings: More (and Less) than Meets the Eye
The Cassini spacecraft is executing a series of maneuvers to raise its orbit above the plane of Saturn’s famous rings. This will offer some breathtaking views that you won’t want to miss. Meanwhile, Cassini scientists are learning surprising things, such as the fact that the most opaque sections of the rings are not necessarily the thickest.
3. Stay on Target
The Juno spacecraft recently completed a course correction maneuver to fine-tune its approach to Jupiter. After years of flight and millions of miles crossed, arrival time is now set to the minute: July 4th at 11:18 p.m. EST. See why we’re going to jupiter HERE.
4. The Many Lives of “Planet X”
The announcement of a potential new planet beyond Neptune creates an opportunity to look back at the ongoing search for new worlds in the unmapped reaches of our own solar system. Review what we’ve found so far, and what else might be out there HERE.
5. Answering the Call of Europa
There are a few places more intriguing that Jupiter’s icy moon, Europa, home to an underground ocean with all the ingredients necessary for potential life. We’re undertaking a new mission to investigate, and the project’s top manager and scientist will be giving a live lecture to detail their plans. Join Barry Goldstein and Bob Pappalardo on Feb. 11 at 10 p.m. EST for a live lecture series on Ustream.
Want to learn more? Read our full list of the 10 things to know this week HERE.
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What do you hope to find on the mars? / What would be the best possible outcome?
The Geminid meteor shower, one of the biggest meteor showers of the year, will peak this weekend, December 13 to 14. We get a lot of questions about the Geminids—so we’ve put together some answers to the ones we’re most commonly asked. Take a look!
The Geminids are pieces of debris from an asteroid called 3200 Phaethon. Earth runs into Phaethon’s debris stream every year in mid-December, causing meteors to fly from the direction of the constellation Gemini – hence the name “Geminids.”
Image Credit: Arecibo Observatory/NASA/NSF
This year, the peak is during the overnight hours of December 13 and into the morning of December 14. Viewing should still be good on the night of December 14 into the early morning hours of the 15th. Weather permitting, the Geminids can be viewed from around midnight to 4 a.m. local time. The best time to see them is around 2 a.m. your local time on December 14, when the Geminid radiant is highest in your night sky. The higher the radiant – the celestial point in the sky from which meteors appear to originate – rises into the sky, the more meteors you are likely to see.
Image Credit & Copyright: Jeff Dai
Find the darkest place you can and give your eyes about 30 minutes to adapt to the dark. Avoid looking at your cell phone, as it will disrupt your night vision. Lie flat on your back and look straight up, taking in as much sky as possible. You will soon start to see the Geminid meteors!
Image Credit: NASA/Bill Dunford
The Geminids are best observed in the Northern Hemisphere, but no matter where you are in the world (except Antarctica), some Geminids will be visible.
Image Credit: Jimmy Westlake
Under dark, clear skies, the Geminids can produce up to 120 meteors per hour – but this year, a bright, nearly full moon will hinder observations of the shower. Still, observers can hope to see up to 30 meteors per hour. Happy viewing!
Image Credit & Copyright: Yuri Beletsky
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