Grizzly bears sighted along the coast of the Hudson Bay have made it into the news in recent years, but did you know they once roamed as far as southern Manitoba too?
Geologic time is truly staggering. It is hard to comprehend even for geologists, so we often rely on analogies to convey the vastness of time. If you could count one year per second, it would take an hour and 17 minutes until you had counted the age of the oldest Egyptian pyramids. Keep going, and it would take over 2 years before you reached the end of the age of dinosaurs. You would have to keep going for another 5 and a half years to get to the age of the earliest dinosaurs and another 12 on top of that to reach the earliest animals. It would be impossible to count to the age of the Earth, as it would take 144 years to get to 4.54 billion.
But, how do we actually know how old a particular specimen or event is? This is one of the most common questions I am asked as Curator of Palaeontology and Geology. It’s an excellent question, but not an easy one to answer in a concise way, so I will do my best to provide a more comprehensive answer here.
Manitoba has changed immensely over Earth’s history. While Churchill is now a cold, arctic environment close to 60 degrees north of the equator, about 450 million years ago it was equatorial and covered by a tropical sea. This is due to the shifting of the plates that make up the Earth’s crust, which move at about the speed that your fingernails grow.
Rocks and Clocks
You may have heard of carbon dating before. This approach relies on the radioactive decay of a naturally occurring form of the chemical element carbon. As with all elements, carbon atoms can come in several different forms, called isotopes. Isotopes share the same number of positive particles (protons) in their atomic nucleus, but differ in the number of neutral particles (neutrons). The majority of carbon on Earth is an isotope called carbon-12, which is stable. However, other forms of carbon exist, including an unstable form called carbon-14, characterized by two extra neutrons in its nucleus. Carbon-14 atoms decay over time, as one of their neutrons converts into a proton, releasing radiation and transforming the unstable carbon atom into a stable nitrogen atom. New carbon-14 is constantly being generated in the atmosphere by the action of cosmic rays from space which cause the conversion of nitrogen atoms into carbon-14.
Critically, the decay of carbon-14 happens at a predictable rate. By measuring this rate, we can predict that half of the carbon-14 that exists now will have decayed in 5,730 plus or minus 40 years. This length of time is known as the half life of carbon-14 and it is this concept that allows us to date materials made of carbon. Living organisms take in carbon, including carbon-14, either from carbon dioxide gas via photosynthesis or from feeding on other organisms. While organisms are alive, their supply of carbon-14 is continuously replenished. Once they die, carbon intake ceases and the carbon-14 “clock” is started. By measuring the amount of carbon-14 remaining in a sample of an ancient organism, we can calculate how long ago it died.
One of the oldest rocks on the surface of the Earth, called Acasta Gneiss, on display in the Earth History gallery. It is close to 4 billion years old and is found in Northwest Territories. The age of the Earth and Solar System are estimated to be even older based on measuring the age of meteorites and samples from the moon, which are less subject to processes that reset the radiometric “clock”.
Unfortunately, there’s a catch: if a sample is more than about 50,000 years old, the amount of carbon-14 remaining will be too small to permit an accurate age estimate. For older samples, scientists have to rely on different elements. For example, uranium-238 decays into lead-206 with a half life of about 4.47 billion years. Since uranium-238 is commonly trapped in in certain minerals when they form, it is ideal for measuring the age of older events in Earth’s history. Several other clocks, or more technically radiometric dating systems, exist and these can often be compared to each other to improve the accuracy of estimates.
Absolute and relative time
Not every sample can be dated using an absolute method. For example, many fossils are too old for carbon dating and have insufficient uranium content for uranium-lead dating (although new approaches are pushing the boundaries of what is possible).
Similarly, sedimentary rocks like sandstones and limestones are formed of many different components including fragments of older rocks, fossils, and mineral crystals that have grown in between. Dating these components can give differing ages, sometimes producing misleading age estimates for samples. Further, alteration of rock under high heat and pressure or by the seeping of groundwater can enable atoms to move into and out of its crystalline structure (element mobility), which can “reset” the radiometric system.
This is where a second, complimentary approach called relative dating comes in. Even before there was a well-developed conception of evolution, scientists noticed that there was a regular pattern to the occurrence of different species throughout Earth’s rock record. We now know that this pattern is a consequence of the evolution and extinction of species. Mammoths, dinosaurs, and trilobites are all found only in particular rock layers and are absent from others. At a finer scale, careful examination reveals multiple successions of particular species, from which a comprehensive sequence can be built up. Since rock layers are deposited one on top of the other, the ordered succession of organisms gives us a clue about the relative age of the layers they are found in. If we can date rock layers above and below a particular fossil using radiometric dating, then we know that the fossil must be intermediate between those ages. If we then find the same fossil elsewhere, we have a relative idea of how old the rock it occurs in must be.
This section of rock on display in the Earth History Gallery is the boundary between the Cretaceous and Paleogene Periods, marking the end of the age of dinosaurs. Radiometric dating has allowed precise age estimates for this boundary layer, recently placing it at 66.02 plus or minus 0.08 million years.
The time scale in the Earth History gallery shows the names of major time intervals. The cylindrical rock slices are pieces of rocks of each interval found in Manitoba. Some time intervals are not represented in our province, corresponding to gaps in the time scale. Since this display was constructed, there have been changes and refinements to the time scale that will require updating in the future.
Fossils are not the only source of information that can be used for relative dating. Chemical and magnetic signatures also exhibit observable patterns of change through time that can be used to order rock layers by age. By combining insights from various relative and absolute dating methods around the world, the Earth’s timescale has been built up. The timescale is broken up into a number of named intervals, often based on particularly noticeable changes in the types of fossils. For example, the end of the Cretaceous Period is marked by the extinction of the dinosaurs, with the exception of birds.
Earth’s geological time scale should certainly be ranked among our most significant scientific achievements. This is the result of a long and fascinating history, with insights being drawn from multiple different disciplines of study around the globe. While we now have a pretty good idea of the age of key events throughout Earth’s history, new research is constantly refining dates, enabling us to understand events in the deep past with ever increasing precision.
Dr. Joe Moysiuk
Curator of Palaeontology & Geology
Joe Moysiuk recently completed his doctoral dissertation at the University of Toronto and Royal Ontario Museum. His expertise centers on the oldest animal fossils and insights they provide about the evolution…
One morning, as she gazes at the starry sky giving way to dawn, a spaceship from outer space crash-lands next to her. On board is Stella, a daring shooting star who urgently needs to find fuel to be able to return to space!
Together, they embark on an exciting quest under the oceans. During their journey, Astéria introduces Stella to the fascinating diversity of marine species, while Stella shares her knowledge about Earth, the Moon, and the Sun. Exploring the deep oceans of Earth and exploring deep space have many similarities, which the two friends discover during their adventure. Gradually, they realize the magical connection that ties underwater life to the vastness of space.
This film, designed for younger viewers, offers authentic underwater visuals that will enchant audiences of all ages. With a fun storyline and endearing characters, the show is appropriate for all ages.
Voyage of the Stars: A Sea and Space Adventure premieres Saturday, March 29 at the Manitoba Museum Planetarium and runs daily during Spring Break programming. It will continue to run weekends starting April 12.
Scott is the Planetarium Astronomer at the Manitoba Museum, developing astronomy and science programs. He has been an informal science educator for thirty years, working in the planetarium and science centre field both at The Manitoba Museum and also at the Alice G. Wallace Planetarium in Fitchburg, Massachusetts. Scott is an active amateur astronomer and a past-President of the Royal Astronomical Society of Canada.
If you live in North America and are set to have clear skies the night of Thursday to Friday, then you’ll have a chance to see a total lunar eclipse this week!
Join Planetarium Astronomer Scott Young to learn how lunar eclipses occur, and when to be on the watch for this one.
Have you heard of Manitoban E. Cora Hind? Renowned agricultural journalist, world traveler, and suffragist, she has a pretty fascinating story! Join Cortney this International Women’s Day to learn more about E. Cora Hind and see some of the objects from her in our collection.
Chris is here to lift our spirits with the science behind Bernoulli’s principle of lift! Join him in the Science Gallery to do a simple experiment that you can try out at home with nothing more than a strip of toilet paper.
March brings the spring equinox, warmer weather, and the last chance to see the winter constellations. This year, March also hosts a pair of eclipses (one visible from North America) and a planetary line-up that is almost as good as it gets.
The Solar System
The “Planetary Parade”: While it’s over-hyped online by people who don’t know the sky very well, this month *is* a good time to spot the planets. In late February and early March, we can see 4 of the 5 bright planets at the same time in early evening. But, it isn’t any more spectacular than it has been for the last month – the planets are effectively always in a “parade”, and so if you didn’t notice it in January or February you might wonder what the fuss is all about. That’s social media for you – anything that reliably generates “likes” or “shares” will be used to drive engagement without managing expectations or even providing accurate content.
Bottom line: you can see most of the planets this month, including Mercury which is generally the hardest one to see because it’s so close to the sun. Enjoy the view!
Mercury reaches its best visibility of 2025 this month, rising into the evening sky at the beginning of the month.
Venus still dominates the western sky at sunset at the beginning of March, but it dives towards the Sun by mid-March. For a few days around its closest conjunction to the Sun, it will be visible in both the morning and evening sky at the same time. See the Sky Calendar for details.
Earth reaches the point in its orbit when its poles are perpendicular to its orbital path around the Sun. We call this occurrence the equinox, and this year the Spring Equinox occurs at 4:01 a.m. Central Daylight Time on March 20, 2025. While this marks the astronomical beginning of spring, it has little connection to the weather. The main event is that the hours of daylight and nighttime are equal – equinox means “equal night”. Any stories about being able to balance an egg on its end only during the equinox are false – you can do that any day of the year, if you have the time and patience for it.
Mars is still bright in the evening sky, forming an ever-changing triangle with the bright stars Castor and Pollux in Gemini. The Moon is nearby on the evening of March 8th.
Jupiter still shines brightly in the evening sky, high in the southwest after sunset in the constellations of Taurus.
Saturn drops into the sunset glare early in the month, and is lost to sight. You *might* catch it in binoculars during the first few days of the month below Mercury, if you have a perfectly flat horizon and crystal-clear skies.
Uranus is to the right of Jupiter, but invisible to the unaided eye. A pair of binoculars will show it as a star-like dot among a sea of other star-like dots; you need a detailed finder chart like those in the RASC Observers’ Handbook to track it down.
Neptune, while technically part of the “parade”, is invisible without a telescope at the best of times, and this month is not the best of times. Neptune is near Venus in the bright twilight sky and probably unobservable this month.
Of the five known dwarf planets, none are visible with typical backyard telescopes this month.
Sky Calendar for March 2025
All times are given in the local time for Manitoba: Central Standard Time (CST) before March 9, and Central Daylight Time beginning at 2:00 a.m. on March 9, 2025. However, most of these events are visible across Canada at the same local time without adjusting for time zones.
Saturday, Mar. 1, 2025 (evening): Mercury begins its two-week period of visibility, rising into the evening sky below Venus. The very thin crescent Moon is nearby on March 1, but likely invisible in the bright sky without binoculars or cameras. (For the “young moon” hunters, it’s a 24-hour-old moon at sunset in Manitoba, close to the limit for what is potentially visible. Flat horizons and clear skies are a must!)
Sunday, Mar. 2, 2025 (evening): The crescent Moon is above Venus in the evening sky, visible to the unaided eye and with glorious Earthshine illuminating the dark side. Photo op!
Monday, March 3, 2025 (evening): The crescent Moon is mid-way between Venus and Jupiter, while Mercury continues to rise higher in the west below Venus.
Wednesday, March 5, 2025 (evening): The Moon and Jupiter form a nice grouping with Aldebaran and the Pleiades star cluster this evening.
Thursday, March 6, 2025 (evening sky): The Moon is above Jupiter, high in the southwest in the evening sky.
Saturday, March 8, 2025 (evening): Starting tonight, the planets Mercury and Venus are visible in the same field of view of typical household binoculars (roughly a 7-degree field). They’ll remain this close until Mercury is lost from sight around March 14.
Also tonight, the Moon is just above Mars high in the southeast after sunset, with the two bright stars Castor and Pollux nearby. Over the course of the night you can see the Moon’s orbital motion as it passes Mars and moves farther away. At 8pm CDT the Moon is right above Mars; by 3am CDT it has moved to be mid-way between Mars and Castor.
Finally, unless you’re up all night, set your non-internet clocks ahead one hour before you go to bed. Daylight Savings Time starts tomorrow at 2am (1:59 a.m. Central Standard Time is followed by 3:00 a.m. Central Daylight Time).
Sunday, March 9, 2025 (morning): Daylight Savings Time started this morning.
Tuesday, March 11, 2025 (evening): Mercury reaches its highest point above the horizon, while Venus has sunk down to almost meet it. After tonight both Mercury and Venus will rapidly sink into the sunset glow.
Thursday, March 13 (evening): The total lunar eclipse begins at 10:57 p.m. CDT tonight and extends throughout the night into early Friday morning. Unlike a solar eclipse, a lunar eclipse is absolutely safe to watch.
Times for the various stages of the total lunar eclipse of March 13-14, 2025. times for Winnipeg, Manitoba, Canada.
Thursday, March 20, 2025: The Vernal Equinox occurs at 4:01 a.m. Central Daylight Time, marking the beginning of astronomical spring. Also on this date, Venus begins to be visible in both the evening and morning skies (see the entry for March 23 for details).
Sunday, March 23, 2025: The Earth passes through the plane of Saturn’s rings. This would afford a rare view of the rings “disappearing”, but unfortunately Saturn will be too close to the Sun for the event to be easily visible.
Also today, Venus passes between us and the Sun (actually, just “above” the Sun from our point of view). For a few days on either side of this, Venus will be visible in both the evening sky after sunset and the morning sky before sunrise before transitioning into a morning-only object.
Saturday, March 29, 2025: There is a partial solar eclipse on this date, but it is only visible from northeastern Canada, Greenland, Iceland, and northwestern Europe. For details on the view from your location, use this link.
Spring break at the Planetarium: Our spring break programming begins Saturday, March 29 and extends through Sunday, April 6, 2025, open daily from 10 a.m. to 4 p.m. Our brand new family show, “Voyage of the Stars: A Sea and Space Adventure” premieres, and we’ll also have an encore presentation of “Edge of Darkness”, which takes us among the dwarf planets such as Ceres and Pluto. Advance tickets and showtimes are available here.
Northern Lights, Meteors, and other Cool Stuff
Outside of the regular events listed above, there are other things we see in the sky that can’t always be predicted in advance.
Aurora borealis, the northern lights, are becoming a more common sight again as the Sun goes through the maximum of its 11-year cycle of activity. Particles from the Sun interact with the Earth’s magnetic field and the high upper atmosphere to create glowing curtains of light around the north (and south) magnetic poles of the planet. Manitoba is well-positioned relative to the north magnetic pole to see these displays often, but they still can’t be forecast very far in advance. A site like Space Weather can provide updates on solar activity and aurora forecasts for the next 48 hours. The best way to see the aurora is to spend a lot of time out under the stars, so that you are there when they occur.,
Random meteors (also known as falling or shooting stars) occur every clear night at the rate of about 5-10 per hour. Most people don’t see them because of light pollution from cities, or because they don’t watch the sky uninterrupted for an hour straight. They happen so quickly that a single glance down at your phone or exposure to light can make you miss one.
Satellites are becoming extremely common sights in the hours after sunset and before dawn. Appearing as a moving star that takes a few minutes to cross the sky, they appear seemingly out of nowhere. These range from the International Space Station and Chinese space station Tianhe, which have people living on them full-time, to remote sensing and spy satellites, to burnt-out rocket parts and dead satellites. These can be predicted in advance (or identified after the fact) using a site like Heavens Above by selecting your location.
Scott Young
Planetarium Astronomer
Scott is the Planetarium Astronomer at the Manitoba Museum, developing astronomy and science programs. He has been an informal science educator for more than thirty years, working in the planetarium and science centre field both at The Manitoba Museum and also at the Alice G. Wallace Planetarium in Fitchburg, Massachusetts. Scott is an active amateur astronomer and a past-President of the Royal Astronomical Society of Canada.
February may be coming to an end, but our love of reading sure isn’t! In this video, our resident Book Girly, Cortney, shows us some of her favourite items in the museum’s book collection – a comic strip series about the life of Louis Riel.
Only a small percentage of the 2.9 million artifacts and specimens in the Museum Collection are able to be displayed at one time. The rest are kept carefully preserved in collections storage, but that doesn’t just mean they’re just piled on shelves or in cupboards out of sight. Everything is carefully stored to ensure its preserved for as long as possible, and for some artifacts that means keeping them cold!
Find out why cold storage is important for preserving certain artifacts in this video with Senior Conservator Carolyn Sirett.