MPLX: High-Yield Distribution Growth Powerhouse Fueled By Excellent Capital Allocation


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Samuel Smith has a diverse background that includes being lead analyst and Vice President at several highly regarded dividend stock research firms and running his own dividend investing YouTube channel. He is a Professional Engineer and Project Management Professional and holds a B.S. in Civil Engineering & Mathematics from the United States Military Academy at West Point and has a Masters in Engineering from Texas A&M with a focus on applied mathematics and machine learning.

Samuel leads the High Yield Investor investing group. Samuel teams up with Jussi Askola and Paul R. Drake where they focus on finding the right balance between safety, growth, yield, and value. High Yield Investor offers real-money core, retirement, and international portfolios. The service also features regular trade alerts, educational content, and an active chat room of like-minded investors.

Perspective: “Do not store up for yourselves treasures on earth, where moth and rust destroy, and where thieves break in and steal. But store up for yourselves treasures in heaven, where neither moth nor rust destroys, and where thieves do not break in or steal; for where your treasure is, there your heart will be also … For what will it profit a man if he gains the whole world and forfeits his soul?” ~ Jesus (Matthew 6:19-21; 16:26)

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Analyst’s Disclosure: I/we have a beneficial long position in the shares of MPLX either through stock ownership, options, or other derivatives. I wrote this article myself, and it expresses my own opinions. I am not receiving compensation for it (other than from Seeking Alpha). I have no business relationship with any company whose stock is mentioned in this article.

Seeking Alpha’s Disclosure: Past performance is no guarantee of future results. No recommendation or advice is being given as to whether any investment is suitable for a particular investor. Any views or opinions expressed above may not reflect those of Seeking Alpha as a whole. Seeking Alpha is not a licensed securities dealer, broker or US investment adviser or investment bank. Our analysts are third party authors that include both professional investors and individual investors who may not be licensed or certified by any institute or regulatory body.



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Recent Reviews


Big sunspots have been few and far between on the sun in recent weeks. But there sure have been lots of smaller ones. On most sunny days I set up a small, filtered telescope to see what the sun’s up to. Solar observing is incredibly fast and easy — telescope, safe filter placed securely over the front lens, tripod, and you’re good to go.

Solar telescope

This is my simple setup for solar observing — 80mm refracting telescope, a solar filter over the front, and tripod.

Contributed / Bob King

On March 16 it looked someone had sprinkled bits of dirt across the sun. I counted 13 different sunspot groups that day using a magnification of 27x. None of them displayed any impressive spots, at least compared to the behemoths of last summer. But their sheer number made an impression.

Sunspots are sites on the sun where magnetic energy is strongly concentrated. They’re dark because they’re about 3,500 degrees cooler than the surrounding 10,000-degree surface. Strong magnetic fields — like those around an ordinary bar magnet but thousands of times more intense — inhibit the flow of hot gases from the solar interior, insulating and chilling the area. Chill is a relative term. Despite their dark appearance, spots are still around 13 times hotter than a very hot oven.

Sunspot group visible UV with whorls and magnet filings S.jpg

An enormous sunspot group from Nov. 2014 is seen in visible light at left. The center view shows the same group in ultraviolet light, and it reveals the whorls of group’s magnetic field. Sprinkle iron filings around a bar magnet (right) and you’ll see similar lines of magnetic force.

Contributed / NASA (left and center), Bob King (right)

At first glance, it may look like the spots are randomly scattered across the sun, but most gather in groups. Some groups stand alone and are easy to tell apart. For others it takes a little experience to see where the border of one ends and a new one starts.

Each group’s members are magnetically linked to each other, with one section acting as the north pole of a magnet, and the other as the south pole. Each bunch is assigned a number so we can keep track of it as the sun slowly rotates on its axis once approximately every 4 weeks.

Astronomers have been counting spots systematically since 1847, but useful data goes back to the early 1600s. Sunspot number is a good indicator of overall solar activity. Flares and coronal mass ejections are frequently connected to sunspot groups, so the more spots — and the more complex sunspot groups become — the better the chances for solar storms to occur. And that means increasing chances to see the northern lights.

Counting them is easy enough, but there’s a twist. Astronomers tally both individual sunspots and groups. Each group is assigned a value of 10 spots. In the photo there are 13 groups, so 13 multiplied by 10 is 130. Next, you add in the number of individual sunspots. I counted 40. Together, the total sunspot number for March 16 comes to 170. That’s a high number and indicative of strong solar activity.

When formally submitting sunspot tallies, an observer also has to multiply their result by a small factor depending on observing conditions and equipment. By counting sunspots with a small, filtered telescope, arriving at what the monthly average is, and plotting the result on a piece of graph paper, the ups and downs of the 11-year solar cycle will appear right before your eyes.

Solar cycle from 1700 to 2025

Counting sunspots reveals the ups and downs of the solar cycle. Sunspot number is shown at left with a timeline along the bottom. Monthly peaks for each cycle are shown in black. Solar Cycle 1 peaked in the year 1761; we’re now in Cycle 25. Notice how sunspot numbers (solar activity) vary from cycle to cycle. The red hump in Cycle 25 is the original prediction, which has been exceeded.

Contributed / NASA, NOAA, ISES

Or you can have the professionals do it. They count sunspots, average monthly numbers and lay it all out on a curve to look for trends. They also study historical patterns and include data like how much radio energy the sun produces, which fluctuates throughout the solar cycle. Before every new cycle they gather and make a prediction of when the next peak, called solar maximum, will occur.

The original forecast for the current cycle, dubbed Cycle 25, was made in 2019 with the peak predicted for this upcoming July. However, more recent forecasts hint that we reached maximum in late 2024, so we may have already passed the peak. A more definitive answer will have to wait until the sun enters a slump. Then we’ll be able to look back with hindsight and better frame the time.

March 21 aurora

A moderate geomagnetic storm hit on Friday night, March 21, lighting up the northern sky with colorful auroras. A stronger storm is expected Saturday night, March 22.

Contributed / Bob King

In the meantime, enjoy the sun’s busy period while you can by catching the northern lights. On Friday night, March 21, we had a fine display in the Duluth region. A stronger storm is forecast for Saturday night, March 22. If the sky stays clear, go out as early as 9 p.m., look north from a dark location, and you might just see arcs and rays dance across the northern sky. I’ll post updates on my Facebook page at facebook.com/astrobobking.

“Astro” Bob King is a freelance writer and retired photographer for the Duluth News Tribune. You can reach him at nightsky55@gmail.com.





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