Amateur Radio Volunteers in Indonesia Link Earthquake Zone with Outside World

ARRL – Following a devastating 7.7-magnitude earthquake and tsunami in Central Sulawesi, Indonesia, on September 28, members of International Amateur Radio Union (IARU) member-society ORARI and other volunteers have been providing emergency communication for community and government interests. The quake and tsunami destroyed the city of Palu, completely cutting power and telephone connections, as well as the cellular communication infrastructure.

New IARU Region 3 Disaster Communication Coordinator Dani Halim, YB2TJV, said Amateur Radio operators in Indonesia immediately responded to the unfolding disaster, establishing an emergency net on 7.110 MHz. Amateur Radio volunteers from other regions also pitched in to support radio communication for emergency news on 7.110 MHz and 7.065 MHz. ORARI has asked that radio amateurs not involved in the emergency response avoid those frequencies. ORARI also activated the LAPAN-ORARI IO-86 satellite as a back-up communication channel. Some radio amateurs with mobile stations have traveled to the affected region to help.

According to Budi Santoso, YF1AR, on Java Island, the local Palu ORARI representative Ronny Korompot, YB8PR, was among the first contacted. Through his mobile station, he reported on conditions and the response, including evacuations. Sutrisno Sofingi, YB8NT, was also heard on 7.110 MHz using an emergency station he assembled at the disaster site. He said Amateur Radio was the only available communication with the outside world.

Amateur Radio also has assisted government agencies following severe damage to the telecommunication infrastructure. Hams operating on 2 meters were communicating information on which roads were open to allow traffic from the outside.

Halim reported that communication was established from the Luwuk Disaster Management Agency some 430 miles from the earthquake’s epicenter to obtain information on landslides and blocked roads and highways.

Salmin Sahidin, YB8IBD, in Southeast Sulawesi has been live streaming audio of the activity on 7.110 MHz via his Facebook page.

The earthquake and subsequent tsunami has claimed upward of 900 lives and caused widespread devastation. Some victims have been reported to be trapped in the debris. The Indonesian National Disaster Mitigation Agency has told news media that, in addition to communication, heavy equipment for rescue operations is limited.  — Thanks to IARU Region 3 and Budi Santoso, YF1AR 

FCC Grants Temporary Request to Permit PACTOR 4 Use in Hurricane Relief

FCC Grants ARRL Temporary Waiver Request to Permit PACTOR 4 Use in Hurricane Relief

ARRL – The FCC has granted an ARRL request for a temporary waiver of Section 97.307(f) of the FCC’s Amateur Service rules to permit the use of PACTOR 4 digital mode for Amateur Radio communication within the continental US related to Hurricane Florence relief. The grant extends through Tuesday, September 18, and a formal order addressing the request for a 30-day waiver will be issued next week, the FCC said.

Section 97.307(f) of the Commission’s Rules limits the digital data emissions of amateur stations operating below 28 MHz to a symbol rate not to exceed 300 baud, and in the 10-meter band (28.0 – 28.3 MHz) to a symbol rate not to exceed 1200 baud, thus precluding the use of PACTOR 4.

PACTOR 4 is a data protocol that permits relatively high-speed data transmission in the HF bands, and many amateur stations active in emergency communications preparedness are capable of using PACTOR 4, which was used to great advantage, pursuant to FCC temporary waivers, in Hurricane Maria relief efforts, and, more recently in preparing for typhoon relief communications in Hawaii.

“ARRL has recently dispatched equipment to the Carolinas and is actively preparing to assist radio amateurs involved with the Amateur Radio Emergency Service and otherwise to conduct disaster relief communications,” ARRL General Counsel Chris Imlay, W3KD, told the FCC in requesting the waiver. The equipment includes PACTOR radio modems with PACTOR 3 and PACTOR 4 capabilities.

ARRL’s request proposed limiting the use of PACTOR 4 to radio amateurs in the Continental US who are directly involved with the hurricane relief efforts involving the US mainland. “This request is without prejudice to the resolution of Docket 16-239 [the so-called “symbol rate” proceeding], which is presently pending and addresses the rule section discussed herein,” Imlay added

IARU Focuses on WRC-19 Preparation and Succession Planning

The Administrative Council (AC) of the International Amateur Radio Union (IARU) held its annual in-person meeting on September 8 and 9, 2018 in Seoul, Republic of Korea, immediately prior to the IARU Region 3 Conference. The AC is responsible for the policy and management of the IARU and consists of the three IARU international officers and two representatives from each of the three IARU regional organizations.

With the 2019 World Radiocommunication Conference (WRC-19) of the International Telecommunication Union (ITU) now little more than a year away, the efforts of two dozen IARU volunteers to defend Amateur Radio’s frequency allocations against commercial pressures and to seek worldwide harmonization of the 50-54 MHz band are reaching a critical stage. Coordination of this team is an ongoing task leading up to the ITU Conference Preparatory Meeting in Geneva in February 2019 and to WRC-19 itself in Sharm El-Sheik, Egypt, in October and November. The work involves presenting the IARU positions on the WRC-19 agenda items to national administrations through the IARU member-societies and actively participating in the ongoing preparations being done in regional telecommunications organizations and the ITU Radiocommunication Sector. The potential for crippling levels of interference to radiocommunications from High Power Wireless Power Transfer (WPT) for electric vehicles is high on the list of concerns.

With these challenges in mind the AC reviewed its strategic plan to develop support for Amateur spectrum allocations and approved the action plan for implementation during the remainder of 2018 and 2019. To resource the plan, the IARU budget for the years 2019-2021 was reviewed and adopted. The budget is based upon anticipated financial contributions from the IARU International Secretariat (IS) and the three regional organizations and reflects ongoing efforts to minimize expenses while maintaining the essential activities for achievement of the plan.

The IARU Constitution and Administrative Council policies define the process for filling the positions of IARU President and Vice President for five-year terms. Member-societies and the three IARU regional organizations are invited to participate in identifying qualified candidates for consideration in a consultative process between the AC and the member-society acting as the International Secretariat (IS), currently the ARRL. This process for the terms of office beginning on May 9, 2019 was initiated at the 2017 meeting of the AC and completed at the 2018 meeting. ARRL President Rick Roderick, K5UR, formally reported that there was consensus that the incumbent President Tim Ellam, VE6SH, and Vice President Ole Garpestad, LA2RR, should be nominated for an additional term. These nominations will be submitted to the IARU member-societies for ratification by mail vote.

Looking to the future, the AC recognized the importance and urgency of succession planning and assigned it an immediate and high priority. Individuals with the qualifications, skills, and willingness to fill volunteer technical and leadership positions must be identified on an ongoing basis in order to maintain the availability of essential personnel resources. Training must be provided so that the volunteer team can function effectively in a rapidly changing regulatory environment.

The growth of Amateur Radio, especially how to attract young people, is a common concern of IARU member-societies. The AC will set out to identify those barriers to growth that the IARU can assist member-societies to address and will encourage member-societies to share successful strategies for growth with one another.

The AC noted with pleasure that considerable progress has been made to develop consistent branding across the IARU and its three regional organizations and thanked the team that has been working on a common design for the four websites. The design was agreed and plans are underway for implementation in the coming months.

The IARU policy on QSL bureaus has been under review for several years. While the IARU QSL bureau system continues to be important for many member-societies and individual Amateurs, escalating expenses represent a growing financial burden for others. Unwanted and undeliverable QSL cards are increasingly recognized as an environmental concern. Possible amendments to the policy continue to be developed for consideration.

In addition to the ITU Radiocommunication Sector the IARU is engaged with the Development Sector, particularly with regard to emergency communication. Additional areas of continuing activity that represent significant effort by volunteer coordinators, advisors, and others include Amateur satellite frequency coordination, electromagnetic compatibility (EMC), and the International Beacon Project. Reports from these coordinators and advisors were received with thanks. The AC agreed to maintain its modest annual financial support of the Beacon Project.

The AC noted the actions taken by the IS and the regions to address the requirements of the General Data Protection Regulation (GDPR) of the European Union and agreed to review its implications on an ongoing basis.

After consideration of several possible alternatives the theme for World Amateur Radio Day, April 18, 2019, was confirmed as “Celebrating Amateur Radio’s Contribution to Society”.

Attending the meeting were IARU President Tim Ellam, VE6SH/G4HUA; Vice President Ole Garpestad, LA2RR; Secretary David Sumner, K1ZZ; regional representatives Don Beattie, G3BJ, Hans Blondeel Timmerman, PB2T, Reinaldo Leandro, YV5AM, Ramón Santoyo, XE1KK, Gopal Madhavan, VU2GMN, and Peter Young, VK3MV. Present as observers were regional executive committee members Jay Bellows, K0QB, Ken Yamamoto, JA1CJP, and Don Wallace, ZL2TLL.

The next in-person meeting of the AC is scheduled to be held immediately prior to the IARU Region 2 Conference in Lima, Peru at the end of September 2019. Virtual AC meetings will be held by teleconference as required.

For more information visit:

ISS Air Leak Fixed

The International Space Station’s (ISS) oxygen breach was contained by NASA and Roscosmos astronauts after the space station began losing air pressure yesterday. The ISS’ cabin pressure is now “holding steady” after ISS Expedition 56 crew members hunted down a breach in the spacecraft’s hull. Alarm bells went off in Houston, Texas, and outside of Moscow on Wednesday, August 29, alerting flight control crews of a pressure drop.

But the six ISS astronauts aboard the ISS were not warned of the space station losing oxygen until the following morning. Both NASA and the European Space Agency (ESA) argued the breach was not dangerous enough to wake the astronauts from their slumber.

NASA said the ISS still had enough oxygen to last the crew for weeks but if the breach had not been sealed, it would have drained the ISS of air in just 18 days. The space agency has now confirmed the breach only caused “a minor reduction of station pressure”.

Yesterday the six astronauts carried out a search in one of the two Russian Soyuz spacecraft modules docked to the orbital laboratory. A minute breach about 2mm in size, smaller than the fingernail on a little finger, was detected in in the upper section of a Soyuz MS-09 spacecraft.

During a live feed broadcast from the ISS a crew controller on Earth was heard saying German astronaut Alexander Gerst had plugged the hole with his finger. The voice said: “Right now Alex has got his finger on that hole and I don’t think that’s the best remedy for it.”

The breach has since been sealed by Roscosmos astronaut Sergey Prokopyev. The Russian astronaut stopped the oxygen leak with a bit of epoxy and cotton gauze after it was first taped over with heat resistant tape.

Flight controllers are now looking into a more permanent patch.

Right now Alex has got his finger on that hole and I don’t think that’s the best remedy for it

NASA Flight Control

Last night NASA said in a statement: “After a morning of investigations, the crew reported that the leak was isolated to a hole about two milimeters in diameter in the orbital compartment, or upper section, of the Soyuz MS-09 spacecraft attached to the Rassvet module of the Russian segment of the station.

“Flight controllers at their respective Mission Control centers in Houston and Moscow worked together with the crew to effect a repair option in which Soyuz commander Sergey Prokopyev of Roscosmos used epoxy on a gauze wipe to plug the hole identified as the leak source.

“As the teams were discussing options, flight controllers in Moscow performed a partial increase of the station’s atmosphere using the ISS Progress 70 cargo ship’s oxygen supply.”

Mission flight control officials are now closely monitoring the space station’s system for additional warning signs.

Russia’s space agency will carry out additional analysis for other leaks.  NASA stressed none of the six astronauts were in any real danger fro the leak.

The space agency told its astronauts “no further action was contemplated for the remainder of the day”.

NASA said: “Flight controllers will monitor pressure trends overnight. “All station systems are stable and the crew is planning to return to its regular schedule of work on Friday.”

 

ARISS Packet System Revives

An Amazing Recovery: ARISS Packet System Revives

ARRL – Similar to the AO-7 satellite resurrection several years ago, the Amateur Radio on the International Space Station (ARISS) packet radio system on the International Space Station (ISS) has begun working again. NASA ISS Ham Radio Project Engineer Kenneth Ransom, N5VHO, said over the weekend that reports he’d received indicated that the NA1SS packet signal returned in mid-August.

“It appears it indeed has started working as of about 11 days ago,” Ransom said. “No idea how long it will last, given the degrading state of the current hardware. The longer it lasts, the better.” Ransom said the revived system will fill the gap until a replacement packet module goes up later this year on a Progress supply vehicle and is installed by the crew on a time-available basis. Satellite enthusiast Patrick Stoddard, WD9EWK, in Arizona reported via the ISS Fan Club site that the ISS packet system was operating on August 25 at 1915 UTC during an 8° pass over the continental US. “I got my position packet through once, no QSOs this pass,” he said in a post.

The packet signal on 145.825 MHz has been copied in Europe, South America, India, and elsewhere. In another August 25 post, Mark Pisani, KK6OTJ, reported copying the packet system during an 18° pass over southern California and said he worked KB6LTY through the system. “Heard over Patagonia Argentina!” Francisco Rodriguez, LU2WBA, enthused in a post on August 24 at 2323 UTC. “Welcome back!” An August 17 post from Marco Antonio, PU2MUS, in Brazil indicated that the system was not active at that time.

Earlier this summer, ARISS hardware team members on the ground reported that they were able to locate a functional duplicate of the ISS packet module that had been in use on the ISS for 17 years before it failed more than a year ago. The packet module has been manifest on the Progress 71P spacecraft launch now set for October 31, with docking on November 2.

ARISS said the subsequent installation will depend on the crew’s busy schedule, but expressed hope that the new packet system hardware could be online again by the end of November.

VA3DBJ.ca Pages Updated

Site Updated

Site updated – The amateur radio page has been updated, with additional information for the International Space Station communications.

The Space/SpaceLodge page, has been added with ISS and other space flight communications information.  More information will be added as time permits. I hope to include SpaceX and Boeing manned space flight information.

ISS

New FCC Part 95 Personal Radio Services Rules Published

New FCC Part 95 Personal Radio Services Rules Published in The Federal Register

Reorganized and updated FCC Personal Radio Services (PRS) Part 95 rules have been published in The Federal Register. Among other things, the PRS covers the Family Radio Service (FRS), General Mobile Radio Service (GMRS), and the Citizens Band Radio Service (CBRS).

The revised rules allot additional FRS channels and increase the power on certain FRS channels from 0.5 W to 2 W. FRS channels are in the 462.5625 – 462.7250 MHz range.

Effective September 30, 2019, it will be illegal to manufacture or import handheld portable radio equipment capable of operating under FRS rules and under other licensed or licensed-by-rule services. The FCC no longer will certify FRS devices that incorporate capabilities of GMRS capabilities or of other services. Existing GMRS/FRS combination radios that operate at power levels of less than 2 W ERP will be reclassified as FRS devices; existing GMRS/FRS radios that operate above that power level will be reclassified as GMRS devices, requiring an individual license.

Radios that can transmit on GMRS repeater input channels will continue to be licensed individually and not by rule.

Once the new rules are effective, CBers will be allowed to contact stations outside of the FCC-imposed — but widely disregarded — 155.3-mile distance limit.

Parker Solar Probe Rockets Toward Sun

NASA’s Parker solar probe rockets toward sun for closest look yet

By Marcia Dunn – The Associated Press – A NASA spacecraft zoomed toward the sun Sunday on an unprecedented quest to get closer to our star than anything ever sent before.

As soon as this fall, the Parker Solar Probe will fly straight through the wispy edges of the sun’s corona, or outer atmosphere, that was visible during last August’s total solar eclipse. It eventually will get within 3.8 million (6 million kilometres) of the surface in the years ahead, staying comfortably cool despite the extreme heat and radiation, and allowing scientists to vicariously explore the sun in a way never before possible.

No wonder scientists consider it the coolest, hottest mission under the sun, and what better day to launch to the sun than Sunday as NASA noted.

“All I can say is, ‘Wow, here we go.’”

“We’re in for some learning over the next several years,” said Eugene Parker, the 91-year-old astrophysicist for whom the spacecraft is named.

Solar encounters

Protected by a revolutionary new carbon heat shield and other high-tech wonders, the spacecraft will zip past Venus in October. That will set up the first solar encounter in November.

Altogether, the Parker probe will make 24 close approaches to the sun on the seven-year, $1.5 billion undertaking.

For the second straight day, thousands of spectators jammed the launch site in the middle of the night as well as surrounding towns, including Parker and his family. He proposed the existence of solar wind – a steady, supersonic stream of particles blasting off the sun – 60 years ago.

It was the first time NASA named a spacecraft after someone still alive, and Parker wasn’t about to let it take off without him. Saturday morning’s launch attempt was foiled by last-minute technical trouble. But Sunday gave way to complete success.

The Delta IV Heavy rocket thundered into the pre-dawn darkness, thrilling onlookers for miles around as it climbed through a clear, star-studded sky. NASA needed the mighty 23-story rocket, plus a third stage, to get the diminutive Parker probe – the size of a small car and well under a ton – racing toward the sun.

From Earth, it is 93 million miles (150 million kilometres) to the sun, and the Parker probe will be within 4 per cent of that distance at its closest. That will be seven times closer than previous spacecraft.

image

“Go, baby, go!” project scientist Nicola Fox of Johns Hopkins University shouted at liftoff.

It was the first rocket launch ever witnessed by Parker, professor emeritus at the University of Chicago. He came away impressed, saying it was like looking at the Taj Mahal for years in photos and then beholding “the real thing” in India.

“I really have to turn from biting my nails in getting it launched, to thinking about all the interesting things which I don’t know yet and which will be made clear, I assume, over the next five or six or seven years,” Parker said on NASA TV.

NASA’s science mission chief, Thomas Zurbuchen, was thrilled not only with the launch, but Parker’s presence.

“I’m in awe,” Zurbuchen said. “What a milestone. Also what’s so cool is hanging out with Parker during all this and seeing his emotion, too.”

Parker, the probe, will start shattering records this fall. On its very first brush with the sun, it will come within 15.5 million miles (25 million kilometres), easily beating the current record of 27 million miles (43 million kilometres) set by NASA’s Helios 2 spacecraft in 1976. Zurbuchen expects the data from even this early stage to yield top science papers.

By the time Parker gets to its 22nd, 23rd and 24th orbits of the sun in 2024 and 2025, it will be even deeper into the corona and travelling at a record-breaking 430,000 mph (690,000 kilometres per hour).

Nothing from Planet Earth has ever hit that kind of speed.

Even Fox has difficulty comprehending the mission’s derring-do.

“To me, it’s still mind-blowing,” she said. “Even I still go, really? We’re doing that?”

Close to the sun

Zurbuchen considers the sun the most important star in our universe – it’s ours, after all – and so this is one of NASA’s big-time strategic missions. By better understanding the sun’s life-giving and sometimes violent nature, Earthlings can better protect satellites and astronauts in orbit, and power grids on the ground, he noted. In today’s tech-dependent society, everyone stands to benefit.

With this first-of-its-kind stellar mission, scientists hope to unlock the many mysteries of the sun, a commonplace yellow dwarf star around 4.5 billion years old. Among the puzzlers: Why is the corona hundreds of times hotter than the surface of the sun and why is the sun’s atmosphere continually expanding and accelerating, as Parker accurately predicted in 1958?

“The only way we can do that is to finally go up and touch the sun,” Fox said.

“We’ve looked at it. We’ve studied it from missions that are close in, even as close as the planet Mercury. But we have to go there.”

The spacecraft’s heat shield will serve as an umbrella, shading the science instruments during the close, critical solar junctures. Sensors on the spacecraft will make certain the heat shield faces the sun at the right times. If there’s any tilting, the spacecraft will correct itself so nothing gets fried. With a communication lag time of 16 minutes, the spacecraft must fend for itself at the sun. The Johns Hopkins flight controllers in Laurel, Maryland, will be too far away to help.

A mission to get close up and personal with our star has been on NASA’s books since 1958. The trick was making the spacecraft small, compact and light enough to travel at incredible speeds, while surviving the sun’s punishing environment and the extreme change in temperature when the spacecraft is out near Venus.

“We’ve had to wait so long for our technology to catch up with our dreams,” Fox said. “It’s incredible to be standing here today.”

More than 1 million names are aboard the spacecraft, submitted last spring by space enthusiasts, as well as photos of Parker, the man, and a copy of his 1958 landmark paper on solar wind.

“I’ll bet you 10 bucks it works,” Parker said.

NIST FY 2019 Budget Would Eliminate WWV and WWVH

UPDATED: White House petition setup. See below.

ARRL – The National Institute of Standards and Technology (NIST) FY 2019 budget request includes shutting down “NIST radio stations in Colorado and Hawaii” — in other words, WWV and WWVH. Radio amateurs, HF listeners, and others around the world routinely make use of the time and frequency standard signals, which also include propagation information. NIST said eliminating funding currently “supporting fundamental measurement dissemination” would include putting WWV and WWVH off the air for a saving of $6.3 million. The overall NIST FY 2019 budget request is $127 million, which, the agency said, is a net decrease of $49 million from FY 2018 levels.

“The proposed reductions will allow NIST to consolidate and focus on narrower core [fundamental] measurement programs while meeting budget levels,” the agency said in its FY 2019 budget summary. “NIST will focus on basic research while reducing funding for efforts applying some of its breakthroughs into new measurement applications.

The FY 2019 proposed budget cuts developed earlier this year came to light via Tom Witherspoon, K4SWL, who maintains The SWLing Post website, after a number of viewers called it to his attention. He posted an article on his blog.

“I’ve always considered WWV and WWVH to be the heartbeat of the shortwaves here in North America — a constant, timely companion and brilliant gauge of HF propagation,” Witherspoon wrote. I assumed both stations would be some of the last to go silent on the shortwaves.”

NIST said other “illustrative” cuts in the FY 2019 budget include:

  • $3.5 million for Lab to Market, which seeks to accelerate technology transfer from federal laboratories
  • $6.6 million in environmental measurements projects across NIST laboratories, including work measuring the impact of aerosols on pollution and climate change, and gas reference materials used by industry to reduce costs of complying with regulations
  • $5.8 million eliminating the NIST Greenhouse Gas (GHG) Measurements program, including Urban Dome research grants to advance the direct measurement of GHG emissions on the scale of cities or regions.
  • $6.7 million in forensic science, reducing the program size to $7.3 million by prioritizing measurement science in the NIST labs and eliminating program management functions and external grants for the Organization of Scientific Area Committees for Forensic Science and the Forensic Science Center of Excellence 
  • $4.1 million in R&D targeting application of NIST quantum breakthroughs to applied measurement needs, including temperature and atmospheric gas metrology

“I find this budget request very disappointing,” Witherspoon said with respect to the proposed elimination of WWV and WWVH. “Let’s hope, somehow, this does not come to fruition.” He said The SWLing Post would be tracking and posting any new developments.

UPDATE: White House petition to maintain NIST funding of WWV time stations.

I recently read your article concerning the proposed shutdown of the NIST stations WWV/WWVH.
To that end, I have gone ahead and created a Whitehouse petition to see if this decision can be reversed:
https://petitions.whitehouse.gov/petition/maintain-funding-nist-stations-wwv-wwvh
Would there be any way you could perhaps post the link to this so that fellow members of the SWLing Post could sign it? I believe the more folks we have sign the better chance we have of maintaining the radio stations we have all come to rely upon.

Tom Kelly

Perseid Meteor Shower 2018

When, Where & How to See It This Weekend

By Sarah Lewin Space.com – According to NASA meteor expert Bill Cooke, the Perseids are perhaps the most popular meteor shower of the year; and in 2018, they’ll be the best shower of the year. During the Perseids’ peak this weekend, spectators should see about 60-70 meteors per hour, but in outburst years (such as in 2016) the rate can be between 150-200 meteors an hour. The meteor shower’s peak will be visible both the nights of Aug. 11-12 and Aug. 12-13, Cooke said, but he’s inclined this year to lean toward the night of Aug. 12-13 for the better show. (Both, however, should be spectacular.)

“This year the moon will be near new moon, it will be a crescent, which means it will set before the Perseid show gets underway after midnight,” Cooke told Space.com. “The moon is very favorable for the Perseids this year, and that’ll make the Perseids probably the best shower of 2018 for people who want to go out and view it.” The Perseids are rich in fireballs, so the show should be even better.

To best see the Perseids, go to the darkest possible location and lean back to observe as much sky as possible directly above you. The rates of Perseids visible will increase from about 10 p.m. in your local time zone all the way through dawn, so the later you can look the better. Earlier in the night there will be fewer meteors, but the ones that appear will have longer tails as they graze along more of the atmosphere. Those in southern latitudes can look toward the northeast to see more meteors.

The 2018 Perseid meteor shower peaks overnight on Aug. 12-13, 2018. This sky map shows where to look at 11 p.m. local time this weekend.
The 2018 Perseid meteor shower peaks overnight on Aug. 12-13, 2018. This sky map shows where to look at 11 p.m. local time this weekend. Credit: Sky & Telescope Magazine

Skywatchers looking out for the Perseids should also be able to see Mars (visible until about 4 a.m. in your local time zone) and Saturn (visible until about 2 a.m. local time); Venus and Jupiter both set before the Perseids are best viewed (9:30 p.m. and 11 p.m., respectively).

Earth will pass through the path of Comet Swift-Tuttle from July 17 to Aug. 24, with the shower’s peak — when Earth passes through the densest, dustiest area — occurring on Aug. 12. That means you’ll see the most meteors in the shortest amount of time near that peak, but you can still catch some action from the famed meteor shower before or after that point.

You can see the Perseid meteor shower best in the Northern Hemisphere and down to the mid-southern latitudes, and all you need to catch the show is darkness, somewhere comfortable to sit and a bit of patience.

What causes the Perseids?

Comet Swift-Tuttle is the largest object known to repeatedly pass by Earth; its nucleus is about 16 miles (26 kilometers) wide. It last passed nearby Earth during its orbit around the sun in 1992, and the next time will be in 2126. But it won’t be forgotten in the meantime, because Earth passes through the dust and debris it leaves behind every year, creating the annual Perseid meteor shower.

The annual Perseid meteor shower occurs when the Earth passes through a stream of dust from the Comet Swift-Tuttle, as shown in this orbit diagram.
The annual Perseid meteor shower occurs when the Earth passes through a stream of dust from the Comet Swift-Tuttle, as shown in this orbit diagram. Credit: Sky & Telescope Magazine

When you sit back to watch a meteor shower, you’re actually seeing the pieces of comet debris heat up as they enter the atmosphere and burn up in a bright burst of light, streaking a vivid path across the sky as they travel at 37 miles (59 km) per second. When they’re in space, the pieces of debris are called “meteoroids,” but when they reach Earth’s atmosphere, they’re designated as “meteors.” If a piece makes it all the way down to Earth without burning up, it graduates to “meteorite.” Most of the meteors in the Perseids are much too small for that; they’re about the size of a grain of sand.

What do you need to see them?

The key to seeing a meteor shower is “to take in as much sky as possible,” Cooke said. Go to a dark area, in the suburbs or countryside, and prepare to sit outside for a few hours. It takes about 30 minutes for your eyes to adjust to the dark, and the longer you wait outside, the more you’ll see. A rate of 60-70 meteors per hour, for instance, means around one meteor per minute, including faint streaks along with bright, fireball-generating ones.

Some skywatchers plan to camp out to see the Perseid meteor shower, but at the very least, viewers should bring something comfortable to sit on, some snacks and some bug spray. Then, just relax and look upward for the celestial show.