April Lyrid Meteor Shower

If you’re a fan of shooting stars, and want to catch bits of Comet Thatcher burn up in the atmosphere, you won’t want to miss the Lyrid meteor shower this April. The Lyrids are one of the oldest known meteor showers, dating back to ancient China and they can produce up to 20 meteors per hour at their peak. The meteor shower is caused by leftover debris from Comet Thatcher, a long period comet (415 year) that has only been observed once since discovery in 1861, and is scheduled to return no earlier than 2283.

But how can you enjoy this celestial spectacle if you live in the city, where light pollution can wash out the night sky? Here are some tips to help you catch a glimpse of the Lyrids this year.

  • The best time to watch the Lyrids is between midnight and dawn on April 22nd to 23rd, when the shower reaches its maximum activity. However, you can also see some meteors a few days before and after this date, as the Earth passes through the debris trail left by comet Thatcher.
  • The Lyrids appear to radiate from the constellation Lyra, which rises in the northeast after sunset and climbs high in the sky by dawn. You don’t need to look directly at Lyra to see the meteors, but it helps to find a spot where you have a clear view over the eastern horizon.
  • To avoid light pollution, try to get away from bright streetlights, buildings, and cars. You can also use an app like Dark Sky Finder or Clear Sky Chart to find a dark location near you. If possible, drive or bike to a park, a hill, or a rural area where you can see more stars. As luck would have it the Moon, only at 10% illumination, will set just before midnight, removing one pesky light source.
  • Once you find a good spot, let your eyes adjust to the darkness for at least 15 minutes. You don’t need any special equipment to watch the Lyrids, just your eyes and some patience. Dress warmly, bring a blanket or a chair, and maybe some snacks and drinks to keep you comfortable.
  • If you’re not too sure where to look, the bright star Vega should help guide you, located East about 45 degrees over the horizon.
  • You can also setup a camera on a tripod with a wide angle lens, taking multiple long exposures of about 20 seconds. Place the radiant of the meteor show on the edge of the frame to capture longer trails.
Lyrid Meteor Shower

Enjoy the show! The Lyrids are known for producing bright and fast meteors, some of which can leave persistent trails in the sky. You might also see some fireballs, which are very bright meteors that can light up the whole sky.

The Lyrid meteor shower is a wonderful opportunity to connect with nature and marvel at the beauty of the cosmos. Don’t let the city lights stop you from experiencing this amazing event. Happy stargazing!

“7 Minutes of Terror”

The folks at JPL created a short film showcasing Perseverance’s critical descent phase for the Mars landing. If everything goes according to plan, we shall have a new rover on Mars at 3:40pm EST on February 18, 2021.

Perseverance is currently “cruising” at 84,600km/h through space with Mars as a target. To give you an idea of what kind of speed that is, here are a few benchmarks:

  • The fastest commercial jet: the Concord flying at Mach 2.04 is just under 2,200km/h
  • Space Shuttle re-entry speed: 28,100km/h
  • Voyager 1, leaving our solar system : 61,500 km/h
  • Parker Solar Probe (fastest man-made object) : +250,000km/h

Perseverance was launched on July 30th, 2020 from Cape Canaveral Air Force Station, Florida, on top of a Atlas V-541 rocket.

Animation of Mars 2020’s trajectory around Sun, Data source: HORIZONS System, JPL, NASA

The only way the rover will be able to decelerate from its current cruising speed is by plunging into the Martian atmosphere at the right angle and using the atmospheric friction to slow it down. That “7 minutes of terror” is the time the rover will spend on re-entry, from approaching Mars at the right angle, to landing in the desired spot on the Martian surface.

Lots of steps need to go right, timed correctly to have a successful landing. Only 22 of the 45 landers sent to Mars have survived a landing. The US is by far the country with the most success (sorry Russia, you’re space program is awesome, but you suck at landing on Mars)

Glancing up at the night sky that February 18, 2021 evening will be very easy to spot Mars, but also the Pleiades star cluster (Messier 45). Mars will be about 5 degrees north of a almost half-illuminated moon. And if you keep looking higher up by 10 degrees you’ll see the famous open star cluster nicknamed the Seven Sisters, also used as the Subaru emblem.

Wide Angle Photography – Perseus

Image

Shooting wide angle long exposures of the sky is always fun, because you never quite know what you will get. On an August night I decided to take a few 20 seconds exposures of the constellation Perseus hoping to catch a few open clusters.  However got surprised by the faint glow of Messier 33 (Triangulum Galaxy) in the photos. This is the furthest object that can be observed to the naked eye, located 2.7 million light years away, and part of the Local Group which includes Andromeda and our Milky Way.

Constellations Perseus and Triangulum (Benoit Guertin)

Constellations Perseus and Triangulum (Benoit Guertin) – CLICK FOR FULL SCREEN

4 x 20 seconds
ISO 6400
17mm F4.0
Canon 80D
August 30, 2019

Ending the Year with Betelgeuse

A few days prior to the holiday break there was news of Betelgeuse dimming to an all-time low, potentially signaling the start of the process that will transform this star into a Supernova. What? Wait a minute… A star in our own galaxy exploding? But that hasn’t been observed since 1604!

Remnant of SN1604 (NASA)

Remnant of SN1604 – last galactic nova (NASA)

There are plenty of novas at any point in time, they just happen to be in galaxies far away (cue Star Wars intro). During those few days or weeks of otherworldly explosions these stars become the brightest object in their host galaxies.

SN2018ivc in galaxy NGC 1068 (Credit: Bostroem et al., 2019.)

SN2018ivc in galaxy NGC 1068 (Credit: Bostroem et al., 2019.)

So if we can see them when they are millions of light years away, what would an exploding star just 700 light years away, like Betelgeuse, look like?

Well if we base ourselves on SN1604 it will be visible to the naked in eye for three weeks, including during daytime. SN1604 was 20,000 light years away, while Betelgeuse is at a fraction of that, so most experts anticipates that it would be as bright as a full Moon.

Now before we go crazy anticipating when Betelgeuse, a red super-giant, will explode, let me present some information to put everything in perspective.

Betelgeuse is a red super-giant of class M1-2 in the constellation Orion, 2nd in brightness just after Rigel. Betelgeuse is one of the largest start we can see when glancing up at the night sky. If Betelgeuse was our Sun, it would engulfed all planets up to Jupiter. Stars of that size aren’t like the nice Smith Ball of fire we imagine our Sun to be. They are more like a loose ball of foam, constantly bubbling and bloating from the incredible heat created in the inner core. If you are starting to think unstable, you are partly right.

Betelgeuse is also a well documented variable star, meaning it periodically varies in brightness.

Recorded Brightness of Betelgeuse Over the Years (credit: AAVSO)

Recorded Brightness of Betelgeuse Over the Years (credit: AAVSO)

So while it is at an all-time low compared to its known ~425 day cycle, it also has a ~5.9 year cycle, and this episode just happens to be a combination of both lows. So no need to panic… for now.

Betelgeuse will one day end as a type II supernovae, probably not for another 100,000 years. Until then we can all glance up during these cold winter nights at how easily the Orion constellation can be spotted and enjoyed. The three bright stars marking the belt and the hour-glass figure is easy to find. Take a few moments to look at Betelgeuse as on a galactic scale it will be gone tomorrow.

Betelgeuse Red Super Giant in Orion (Benoit Guertin)

Betelgeuse Red Super Giant in Orion (Benoit Guertin)

Coming this March – Reentry of Chinese Space Station

Its inevitable, what goes up must come down. On average there is one large piece of equipment that re-enters our atmosphere every week. Some are controlled and planned decommissioning of satellites after their useful life. They are purposely commanded for re-entry and burn-up in the atmosphere to avoid adding debris to our already crowded space orbits or worse, cause a collision with another satellite creating an enormous field of debris. Other objects that re-enter are left to fall on their own such as discarded rocket bodies and old satellite that ceased to operate long ago or malfunctioned and can no longer be controlled.

Tiangong-1 : First Chinese space station launched in 2011

Tiangong-1 : First Chinese space station launched in 2011

This coming March the 8,500kg (18,700lbs) Tiangong-1 Chinese space station is coming back to Earth. Launched in September 2011 and used for two manned missions, it suffered a malfunction and the Chinese have not been in control of it since 2016. The space station has been in a decaying orbit ever since, and now below the 300km altitude  where Earth’s atmosphere is causing the space station to slow down due to aerodynamic drag it will soon make its re-entry.

Delta 2 rocket fuel tank surviving re-entry near Georgetown, TX, on 22 January 1997

Delta 2 rocket fuel tank surviving re-entry near Georgetown, TX, on 22 January 1997

Now there is no need to panic. Most of Earth is ocean, and we’ll probably not see anything let alone have a piece of it land in a city. However as this is a fairly large body, there is a good chance  not all pieces will burn up and some may make it to the surface.

This isn’t the first time a space station makes a re-entry.  The American Skylab at 77 tons re-entered in 1979, and Russian Mir (120 tons) made its re-entry in 2001.
For the Mir re-entry, Taco Bell even got it onto the re-entry buzz by anchoring a large

Taco Bell target for Mir re-entry (2001)
Taco Bell target for Mir re-entry (2001)

target off the Australian coast along the planned re-entry track, and should Mir crash into it there would be free tacos for all Americans. The fast food chain even took out an insurance policy just in case it would happen.

In early January 2018, Tiangong-1 is orbiting at an altitude of around 270-290km (to put that into perspective, ISS is at a 400km orbit) and in a 45 deg orbit, hence the re-entry will be within those latitudes.  The green area in the map below is where Tiangong-1 could make a re-entry, and also marks where the re-entry could be observed.

Tiangong-1 ground coverage - http://www.aerospace.org

Tiangong-1 ground coverage – http://www.aerospace.org

It’s still too early to determine the time and location of potentially crash site, as Earth’s atmosphere is influenced by space weather and swells based on our Sun’s moods, which alters the drag force on the space station.  However various space centers and organizations will continue to track the space station the coming weeks to improve the prediction.

You can follow everything at Aerospace.org for up to date information and predictions.

What could the re-entry look like?  Below is a video shot by NASA of the Japanese Hayabusa spacecraft during a controlled re-entry on June 13, 2010

Red Dwarf Spaceship Spotting?

The big news this week is the first recordings and observations of an interstellar object.  Of the 750,000 asteroids and comets that have been cataloged up to now, every one of them originate from within our solar system. This object detected by the Pan-STARRS1 telescope and named A/2017 U1 or “Oumuamua”, a Hawaiian word for scout or messenger from the distant past, came from another part of our galaxy. Based on measurements made from multiple ground-based telescopes it is believed to be rather long and of a deep red color . Below is an artist’s rendering of this extra-solar visitor. While a comet would have generated some type of coma or tail travelling near the Sun, no such activity was recorded, hence it’s believed to be an asteroid-type object.

Artist’s impression of the interstellar asteroid `Oumuamua

Credit: ESO/M. Kornmesser

 

 

 

 

 

Measurements over multiple nights allowed to establish the trajectory, which clearly shows that it did not originate from the Oort cloud or other asteroid/comet rich fields surrounding the Sun. While the discovery was made only on an October 19 image, its closest approach to the Sun was September 9th.

eso1737b

Diagram showing the trajectory of A/2017 U1 (ESO/K. Meech, et al.)

Now I thing they got it all wrong.  What they picked-up was the Red Dwarf mining ship swinging by our neighborhood!

RedDwarfShip

Red Dwarf mining vessel owned by the Jupiter Mining Corporation (BBC)

 

ESO Press Release

Animation – Movement of Comet 41P

The word “planet” comes from the Greek work “planan” which means to wander. Early star gazers noticed that some bright stars moved with respect to other fixed stars.  Those bright stars are our closest planets: Mercury, Venus, Mars, Jupiter and Saturn. Comets also move a fair bit across the sky, but the origin of the word has more to do about stars “with long hair” than it’s traveling behavior.

Last weekend I managed to photograph comet 41P//Tuttle–Giacobini–Kresák, and I identified in my blog that it’s movement was visible frame to frame. Well I’ve finally gotten around to create a small animation of that movement. For those wondering what’s the comet’s velocity, it’s currently travelling at 37.4 km/s.

Animation of comet 41P/Tuttle–Giacobini–Kresák (45 minutes)

Animation of comet 41P/Tuttle–Giacobini–Kresák (41 minutes)

The above is composed of 32 frames, each a 1 minute exposure spanning a time of 41 minutes. You are probably thinking “it should be 32 minutes, not 41!”. That is because I have a delay between each frame to allow the camera to send the photo to the computer. Hence between the first and last frame, 41 minutes have elapsed.

Large Asteroid to Pass Near Earth

On April 19th a considerable sized asteroid will pass about 4.6 lunar distances (1.8 million km) from Earth.  While there is no chance of it impacting our planet, this 650m asteroid was only discovered three years ago, and it will be the closest encounter of a large asteroid since asteroid Toutatis in September 2004. The next predicted fly-by of a large asteroid is 2027 with 800m wide 1990 AN10.

The expected magnitude could reach up to 11 during the close approach, hence a decent sized scope will be required, and due to the rapid movement may be hard to locate and track.

Sky chart for asteroid 2014 JO25 covering April 18th to 20th 2017

And as a bonus, comet PanSTARRS (C/2015 ER61) will also make its closest approach to Earth on the 19th, but 10 times farther away as the asteroid.  I should be visible with small telescopes or binoculars in the constellation Aquarius in the dawn sky.

Source: NASA/JPL

Comet 41P/Tuttle-Giacobini-Kresak

Periodic comet 41P/Tuttle-Giacobini-Kresak is currently a magnitude 8 object for telescopes and unlike many other current bright comets like C/2015 ER61 (PANSTARRS) and C/2017 E4 (Lovejoy) it is visible for a good portion of the night while the other two are only visible in the morning twilight for those like me in the northern hemisphere.

On April 13th comet 41P was in the constellation Drago, which is where I managed to photograph it.

Comet 41P/Tuttle-Giacobini-Kresak (13-Apr-2017) - Benoit Guertin

Comet 41P/Tuttle-Giacobini-Kresak (13-Apr-2017) – Benoit Guertin

Not much of a tail on this comet, and I’ve checked other photos taken with larger scopes and the result is also just a coma around the nucleus.

Because it is passing near Earth, its movement in the sky is quite noticeable frame-to-frame in the captured images. For the registration and stacking with comets, this is done by alignment on the comet and not the stars, hence the star trails in the above image. I performed another stacking, this time using the stars to align, and the comet’s movement becomes obvious. The displacement measures 2.6 arc-minutes in the 41 minutes that elapsed between first to last exposure.

UPDATE: Created a short video showing the comet’s movement

Distance traveled by the comet in 41 minutes

Distance traveled by the comet in 41 minutes

My setup was less than ideal, as the constellation was only visible from the front of my house.  Yes that is a lovely street-light shining right across the street.  Luckily the telescope was pointing a little to the right, and a rolled piece of cardboard help act as an dew-shield extension to block the glare.  But on the good side I had a nice solid concrete surface and got a very good polar alignment with 1 minutes exposures giving me nice round stars.  Hmmm, might explore this setup a little more often…

Setup in the garage to image comet in constellation Drago

Setup in the garage to image comet in constellation Drago

Telescope: SW80ED
Camera: Canon XTi (450D)
Exposure: 32 x 60sec ISO 800
DeepSkyStacker, IRIS, GIMP

Other comets of interest for 2017

EXOPLANET SERIES – TRAPPIST-1

On Wednesday NASA made headlines by announcing that researchers had detected seven exoplanets orbiting a dim dwarf star.  These exoplanets are determined, based on measurements, to be approximately Earth-sized solid planets and three happen to fall in the “Goldilocks Zone” where water could exist in liquid form; not too hot, not too cold.  Lots of people started speculating that in a few years we’ll find out if one of those planets harbors life.  However that is just plain crazy-talk.  The importance of this discover is that complex exoplanet systems do exist; the Solar System is not an exception, and that life is also not an exception.

The TRAPPIST-1 system

The TRAPPIST-1 system contains a total of seven planets, all around the size of Earth. Three of them — TRAPPIST-1e, f and g — dwell in their star’s so-called “habitable zone.” [NASA/JPL]

 

0.60m Ritchey-Chrétien Reflector [TRAnsiting Planets and PlanetesImals Small Telescope–South / ESO]

0.60m Ritchey-Chrétien Reflector [TRAnsiting Planets and PlanetesImals Small Telescope–South / ESO]

The TRAnsiting Planets and PlanetesImals Small Telescope–South made the discovery back in May 2016 of three exoplanets around the small star.  But it was with the help of larger telescopes and the space-based Spitzer telescope that the count increased to seven and their orbits could be confirmed.  What I find interesting is the initial discover was done by a relatively “small” 0.60m telescope.  OK not your typical backyard astronomy gear, but scale that down by 1/3 and you have equivalent optics for about $3000.  Add a mount and CCD and for $10,000 you could probably have your very own exoplanet hunter!

Back to the crazy-talk of finding life in this exoplanet system… Anyone who has studied the history and formation of the Solar System knows that there have been a series of unlikely events that have led to where we are today.  Starting with the Sun, probably a 3rd generation star, where heavy elements like Calcium and Iron necessary for life as we know it were produced by previous stars and supernovas that used to exist in this spot of the galaxy we now occupy.  All elements beyond Hydrogen are produced by stars, either through fusion or when they dramatically explode as supernovas.  The atoms making up the air, the trees, the oceans, ourselves were not created in our Solar System during its formation.  The Sun is currently only generating Helium and Lithium out of Hydrogen through the wonders of fusion.  All the heavier atoms within us were created by previous stars that no longer exist.  Hence for solid Earth-like exoplanets to exists there needs to have been one to two previous generation of stars in the region.

An alien race observing our Solar System would surely first spot Jupiter.  One could almost say that it characterizes our home in this part of the galaxy.  With its strong gravity this gas giant plays the vital role of neighborhood vacuum cleaner.  It is either mopping up or launching away asteroids and comets that would otherwise impact Earth, bringing relative calm to the inner Solar System.  If Earth was constantly bombarded by solar objects, there is no way that life could suitably evolve from slimy unicellular organisms.  It took 3 billion years for multi-cellular organisms to show up once life appeared on Earth.  If cataclysmic comet and asteroid impacts are a frequent occurrences, then there is little chance that complex organisms would come to be.

Looking at another element, TRAPPIST-1 is described as an ultra-cool dwarf star just shy of 40 light years from Earth in the constellation Aquarius.  If we forget that it’s a fraction of our Sun’s size and brightness (hence heat generation), it is relatively young at 1 billion years old.  So while there may be three planets that could be habitable, life may not have even begun yet.  Our own Sun is 4.3 billion years old, and the animals we see around us have only been around for the last 14-16 million years.  So what could be in a 1 billion year old planetary system? Assuming all the ingredients are there for life to exist, you probably only have bacterial soup.

Now, my article was getting long, and I wanted to cover many more subjects, too many for a single article.  Hence I’ve decided to break them out into the EXOPLANET SERIES and will publish them over time.