Garcelle Feuds With Boz and Dorit


RHOBH Reunion Spoilers: Garcelle Beauvais Feuds With Boz & Reignites Convo Over Dorit’s Home Invasion, Plus Morgan Wade Drama, and Find Out If Sutton Apologized to Dorit as Garcelle Didn’t Partake in Group Pic

Credit: Instagram

According to a new report, at the upcoming Real Housewives of Beverly Hills reunion, Garcelle Beauvais reignited talks about Dorit Kemsley’s home invasion, and she was displeased when Bozoma Saint John defended Dorit. At the taping, Sutton Stracke allegedly apologized to Dorit, and Garcelle didn’t participate in the group photo at the end.

Early in the season, Garcelle suggested that “someone” perhaps plotted against Dorit before her 2021 home invasion. Some fans believe she was insinuating that Dorit’s husband PK Kemsley was involved. PK, who’s now separated from Dorit, later wrote a post shading Garcelle, and he suggested she should find a better way to make money.

According to sources speaking to Reality Scoop, Sutton apologized to Dorit at the reunion for her disses about Dorit’s money.

The sources also claimed that Garcelle restarted the discussion about Dorit’s home invasion, and Boz came to Dorit’s defense. This reportedly displeased Garcelle, who seemingly expected Boz to back her up when tensions arose. The insiders claimed that Garcelle didn’t join the group for the cast photo at the reunion’s conclusion.

Additionally, Garcelle reportedly pressed Kyle Richards to address rumors about her friendship with Morgan Wade. But the conversation was soon shut down — by either Kyle or someone else.

Last month, Boz reflected on her choice to question Kyle about her texts with PK amid his separation with Dorit. At the time, Garcelle gave Boz the information about the texts.

“Garcelle gave me the charge,” said Boz in an interview for Access Hollywood‘s Housewives Nightcap. “She came over and told me, and she knew that I couldn’t just let it be. I think I was used in that moment because I’m also like, ‘Garcelle, why didn’t you go and tell everybody?’ She could’ve called Dorit and told her, but she came and told me, and then I had to go do it.”

She also seemed to call out Kyle and Garcelle for having an issue with her and Dorit’s friendship.

“I’m giving [Dorit] advice … as a friend does. Is there a timeline by which you’re allowed to then give advice to somebody, or are you just supposed to stay quiet? Even if you see your friend facing down an oncoming train, you’re just supposed to stand there and watch them?” she explained. “If I’m not here, which one of you is gonna be talking to her? Which one of you is going to be supporting her? None of you.”



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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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