The only pivot they know is the quote from Friends

I am an engineer so take what you like from that information. I know the stereotype well but the best business leaders I've ever worked with directly were good engineers before they were anything else. I don't think it's possible to have a sustainable business plan without a rigorous understanding of every part of the process of making whatever it is that you're selling. There isn't anyone out there who knows that better than the engineers who design and build it.

It’s just not their passion to deal with legalities, OSHA, taxes, payroll, accounts payable, accounts receivable, etc.

All of that should be handled by lawyers, accountants, and finance people. The MBA is not generally the one doing any of that directly though. They're the ones managing the people that do that work and telling them what to prioritize. And therein lies the problem as you correctly pointed out; those are all secondary business functions. They are important parts of any business but are not the fundamental driver of any real business. What the company makes or sells or consults about or whatever else is the actual business and MBAs don't generally know a thing about that part. Letting them steer all of the corporate ships in America is a huge miscalculation and it's also a big part of why things are getting more and more fucked up for everybody.

They aren’t looking at the human factor at all.

That is an important point. It's also a pretty good summary of the problem. MBAs ignore everything that made a business successful (people being a huge factor here) and focus on eternally increasing profits, which inevitably leads to making the product as shitty as it can possibly be while still somewhat meeting expectations, and even that last part is becoming less and less important.

Millenials were forced to go to Darren Group restaurants and Applebee's almost exclusively growing up.

Blocking advertising isn't what hurt them with millenials, it's an entire childhood of awful food.

The Thai Union owns 49% of the stock. That shouldn't be enough to control the company, but the fact that "none" of the C suite agreed with getting rid of the other suppliers but it happened anyway?

Maybe. Perhaps Thai Union was going for vertical integration and wanted to have control of the fried shrimp lifecycle all the way to your mouth, but bit off more than they could chew.

Before the Sun goes cold, it will enter a red giant stage which will bake and then envelop Earth.

https://en.wikipedia.org/wiki/Sun

The Sun does not have enough mass to explode as a supernova. Instead, when it runs out of hydrogen in the core in approximately 5 billion years, core hydrogen fusion will stop, and there will be nothing to prevent the core from contracting. The release of gravitational potential energy will cause the luminosity of the Sun to increase, ending the main sequence phase and leading the Sun to expand over the next billion years: first into a subgiant, and then into a red giant.[139][142][143] The heating due to gravitational contraction will also lead to expansion of the Sun and hydrogen fusion in a shell just outside the core, where unfused hydrogen remains, contributing to the increased luminosity, which will eventually reach more than 1,000 times its present luminosity.[139] When the Sun enters its red-giant branch (RGB) phase, it will engulf (and very likely destroy) Mercury and Venus. According to a 2008 paper, Earth's orbit will have initially expanded to at most 1.5 AU (220 million km; 140 million mi) due to the Sun's loss of mass. However, Earth's orbit will then start shrinking due to tidal forces (and, eventually, drag from the lower chromosphere) so that it is engulfed by the Sun during the tip of the red-giant branch phase 7.59 billion years from now, 3.8 and 1 million years after Mercury and Venus have respectively suffered the same fate.[143]

By the time the Sun reaches the tip of the red-giant branch, it will be about 256 times larger than it is today, with a radius of 1.19 AU (178 million km; 111 million mi).[143][144] The Sun will spend around a billion years in the RGB and lose around a third of its mass.[143]

After the red-giant branch, the Sun has approximately 120 million years of active life left, but much happens. First, the core (full of degenerate helium) ignites violently in the helium flash; it is estimated that 6% of the core—itself 40% of the Sun's mass—will be converted into carbon within a matter of minutes through the triple-alpha process.[145] The Sun then shrinks to around 10 times its current size and 50 times the luminosity, with a temperature a little lower than today. It will then have reached the red clump or horizontal branch, but a star of the Sun's metallicity does not evolve blueward along the horizontal branch. Instead, it just becomes moderately larger and more luminous over about 100 million years as it continues to react helium in the core.[143]

When the helium is exhausted, the Sun will repeat the expansion it followed when the hydrogen in the core was exhausted. This time, however, it all happens faster, and the Sun becomes larger and more luminous. This is the asymptotic-giant-branch phase, and the Sun is alternately reacting hydrogen in a shell or helium in a deeper shell. After about 20 million years on the early asymptotic giant branch, the Sun becomes increasingly unstable, with rapid mass loss and thermal pulses that increase the size and luminosity for a few hundred years every 100,000 years or so. The thermal pulses become larger each time, with the later pulses pushing the luminosity to as much as 5,000 times the current level. Despite this, the Sun's maximum AGB radius will not be as large as its tip-RGB maximum: 179 R☉, or about 0.832 AU (124.5 million km; 77.3 million mi).[143][146]

Models vary depending on the rate and timing of mass loss. Models that have higher mass loss on the red-giant branch produce smaller, less luminous stars at the tip of the asymptotic giant branch, perhaps only 2,000 times the luminosity and less than 200 times the radius.[143] For the Sun, four thermal pulses are predicted before it completely loses its outer envelope and starts to make a planetary nebula. By the end of that phase—lasting approximately 500,000 years—the Sun will only have about half of its current mass.[citation needed]

The post-asymptotic-giant-branch evolution is even faster. The luminosity stays approximately constant as the temperature increases, with the ejected half of the Sun's mass becoming ionized into a planetary nebula as the exposed core reaches 30,000 K (29,700 °C; 53,500 °F), as if it is in a sort of blue loop. The final naked core, a white dwarf, will have a temperature of over 100,000 K (100,000 °C; 180,000 °F) and contain an estimated 54.05% of the Sun's present-day mass.[143] The planetary nebula will disperse in about 10,000 years, but the white dwarf will survive for trillions of years before fading to a hypothetical super-dense black dwarf.[147][148] As such, it would give off no more energy for an even longer time than it was a white dwarf.[149]

True, it'll get you, what, fries and half a drink?