Me Nutrition

🍝 Rigatoni Carbonara

Origin: Italy · Lazio (Rome)
608kcal
per serving · 320 g
190kcal
per 100 g
29 gProtein9 g / 100 g
27 gFat8.5 g / 100 g
74 gCarbs23 g / 100 g

Rigatoni carbonara is the Roman classic made with short ridged pasta: crisp guanciale, eggs, pecorino romano and lots of black pepper. The hot pasta gently cooks the egg and cheese into a glossy, creamy coating without any cream. It is salty, peppery and rich, and is eaten immediately while the sauce is silky.

Diets

✕
Not vegetarianbecause of: guanciale
✕
Not veganbecause of: guanciale, egg, pecorino
✕
Contains porkbecause of: guanciale
✕
Contains glutenbecause of: rigatoni pasta
✕
Contains dairybecause of: pecorino
✕
Not keto23 g carbs per 100 g

Allergens

Contains (in a typical recipe):

What it is made of

rigatoni pastaguancialeeggpecorinoblack pepper

Recipe

4 servings20 min

Ingredients

Method

  1. Cook the guanciale in a dry pan until crisp and take the pan off the heat.
  2. Whisk the yolks, egg, pecorino and plenty of pepper into a thick cream.
  3. Boil the rigatoni until al dente and add it to the guanciale.
  4. Away from the heat, stir in the egg mixture with a few spoons of pasta water until creamy, then serve.

How to make it lighter

History

Carbonara is first documented in Italy in the years after the Second World War, and its exact origin is debated; one popular theory links it to supplies of eggs and bacon brought by American troops. Rome claims the dish, and rigatoni is one of the shapes commonly used there besides spaghetti.

Count it in one photo

Point your camera at the table — Me Nutrition recognises Rigatoni Carbonara and every other dish, with calories and macros for each. Ate only half? Slide it.

Download on the App Store

Similar dishes

Values are estimates per 100 g for a typical recipe; home and restaurant versions vary. Diets and allergens are worked out from the ingredients of a typical recipe — always check with whoever cooked the dish. Not medical advice. Nutrition data: Me Nutrition dish database v13. How we count →